Abstract
The description of the tempo-spatial evolution of the composition of cosmic gas on galactic scales is called ‘galactic chemical evolution’. It combines the knowledge about cosmic sources of nuclei (that is their internal workings and nucleosynthesis yields, and their properties such as frequency of occurrence and spatial distribution), with knowledge about the formation and evolution of these sources in the greater context of a galaxy, as well as transport processes of gas within galaxies. It provides a useful framework, allowing us to interpret the large amount of observational data concerning the chemical composition of stars, galaxies and the interstellar medium.
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Notes
- 1.
Stars of the Galactic disk with ages comparable to, or much younger than, the Sun (4.5 Gy) are called Population I. They are the only stellar population which contains massive (hence short-lived) stars observable today. Stars of the Galactic halo are much older (> 10 Gy) and are called Population II.
- 2.
In principle, the IMF may depend on time, either explicitly or implicitly (i.e. through a dependence on metallicity, which increases with time); in that case one should adopt a Star Creation Function C(t, M) (making the solution of the GCE equations more difficult). In practice, however, observations indicate that the IMF does not vary with the environment, allowing to separate the variables t and M and adopt C(t, M) = Ψ(t)Φ(M).
- 3.
Massive stars also eject part of their mass through a wind, either in the red giant stage (a rather negligible fraction) or in the Wolf-Rayet stage (an important fraction of their mass, in the case of the most massive stars).
- 4.
This is the so called Instantaneous Mixing Approximation, not to be confused with the Instantaneous Recycling Approximation (IRA), to be discussed in Sect. 11.1.3.3.
- 5.
An exception to that rule is fragile D, already burned in the Pre-Main Sequence all over the star’s mass; Li isotopes are also destroyed, and survive only in the thin convective envelopes of the hottest stars.
- 6.
Schmidt (1959) describes the distributions of gas and young stars perpendicularly to the galactic plane (z direction) in terms of volume densities ρ Gas ∝ exp(−z∕h Gas) and ρ Stars ∝ exp(−z∕h Stars) with corresponding scaleheights (obervationally derived) h Gas=78 pc and h Stars=144 pc∼2 h Gas; from that, Schmidt deduces that \(\rho _{Stars} \propto \rho _{Gas}^2\), that is N=2.
- 7.
Metallicity dependent lifetimes have to be taken into account in models of the spectrophotometric evolution of galaxies, where they have a large impact. In galactic chemical evolution calculations, they play an important role in the evolution of s-elements, which are mostly produced by long-lived AGB stars of ∼1.5–2 M⊙.
- 8.
LIMS are defined as those stars evolving to white dwarfs. However, there is no universal definition for the mass limits characterizing Low and Intermediate Mass stars. The upper limit is usually taken around 8–9 M⊙, although values as low as 6 M⊙ have been suggested (in models with very large convective cores). The limit between Low and Intermediate masses is the one separating stars powered on the Main Sequence by the p-p chains from those powered by the CNO cycle and is ∼1.2–1.7 M⊙, depending on metallicity.
- 9.
In active galaxies the central supermassive black hole also plays a role, and even dominates over the impact from massive stars for central regions, and for entire galaxies in late (largely-processed) evolution such as at low redshifts.
- 10.
In this book we only address the scales and processes within a galaxy, as it is driven by massive stars and can be traced by radioactive material; in this and further sections of this chapter, the broader (cosmic evolution) context is also relevant.
- 11.
AGB stars form colorful planetary nebulae, massive-star winds form gas structures within the HII-regions created by the ionizing radiation of the same stars, and thus a similarly-rich variety of colorful filamentary structure from atomic recombination lines results. Supernova remnants are the more violent version of the same processes.
- 12.
Feedback from supermassive black holes is small by comparison, but may become significant in AGN phases of galaxies and on the next-larger scale (clusters of galaxies, see (e)). Galaxy interactions and merging events are also important agents over cosmic times, their overall significance for cosmic evolution is a subject of many current studies.
- 13.
Gaseous flows in the plane of a galactic disk, due e.g. to viscosity, are called inflows; for simple GCE models they also constitute a form of infall.
- 14.
Alternatively, the theory of general relativity may fail at small accelerations.
- 15.
In fact, it is difficult to account for the chemical and kinematical properties of all three galactic components in the monolithic collapse scenario.
- 16.
G-type stars are bright enough for a reasonably complete sample to be constructed and long-lived enough to survive since the earliest days of the disk; the same problem is encountered if F- or K- type stars are used.
- 17.
In fact, the data can be corrected for scaleheight effects only in the framework of a model of the vertical dynamical equilibrium of the local disk, which requires as input the “weight” of each stellar population as a function of its metallicity, i.e. a chemo-dynamical model of GCE is required. Thus, the best approach consists, not in comparing the GCE model with the corrected data, but in (a) calculating the local vertical structure by using the GCE data (surface density vs metallicity) as input, (b) correcting the GCE model metallicity distribution (which refers to the total surface area of the local cylinder), by taking into account the vertical disk structure calculated in (a), and finally (c) comparing the corrected MD of the GCE model to the original (local volume) data. Such an approach is used e.g. Sommer-Larsen and Dolgov (2001).
References
Armstrong JW, Rickett BJ, Spangler SR (1995) Electron density power spectrum in the local interstellar medium. Astrophys J 443:209–221. https://doi.org/10.1086/175515
Audouze J, Tinsley BM (1976) Chemical evolution of galaxies. Annu Rev Astron Astrophys 14:43–79. https://doi.org/10.1146/annurev.aa.14.090176.000355
Beck R (2008) Galactic and extragalactic magnetic fields. In: American Institute of Physics conference series, vol 1085, pp 83–96. https://doi.org/10.1063/1.3076806
Bell EF, Zucker DB, Belokurov V, Sharma S, Johnston KV, Bullock JS, Hogg DW, Jahnke K, de Jong JTA, Beers TC, Evans NW, Grebel EK, Ivezic Z, Koposov SE, Rix HW, Schneider DP, Steinmetz M, Zolotov A (2007) The accretion origin of the milky way’s stellar halo. ArXiv e-prints 706, 0706.0004
Beuermann K, Kanbach G, Berkhuijsen EM (1985) Radio structure of the galaxy - thick disk and thin disk at 408 MHz. Astron Astrophys 153:17–34
Bienaymé O, Soubiran C, Mishenina TV, Kovtyukh VV, Siebert A (2006) Vertical distribution of galactic disk stars. Astron Astrophys. arXiv:astro-ph/0510431
Binney JJ, Evans NW (2001) Cuspy dark matter haloes and the Galaxy. Mon Not R Astron Soc 327:L27–L31. https://doi.org/10.1046/j.1365-8711.2001.04968.x, astro-ph/0108505
Blitz L, Rosolowsky E (2006) The role of pressure in GMC formation II: the H2-pressure relation. Astrophys J 650:933–944. https://doi.org/10.1086/505417, astro-ph/0605035
Boissier S, Prantzos N (1999) Chemo-spectral evolution of the milky way and of spiral disks. Astrophys Space Sci 265:409–410. https://doi.org/10.1023/A:1002181826858
Boulanger F, Perault M (1988) Diffuse infrared emission from the galaxy. I - solar neighborhood. Astrophys J 330:964–985. https://doi.org/10.1086/166526
Boulanger F, Abergel A, Bernard JP, Burton WB, Desert FX, Hartmann D, Lagache G, Puget JL (1996) The dust/gas correlation at high Galactic latitude. Astron Astrophys 312:256–262
Breitschwerdt D (2001) Modeling the local interstellar medium. Astrophys Space Sci 276:163–176
Breitschwerdt D (2004) Self-consistent modelling of the interstellar medium. Astrophys Space Sci 289:489–498. https://doi.org/10.1023/B:ASTR.0000014982.31688.bf, arXiv:astro-ph/0303237
Brown JC, Haverkorn M, Gaensler BM, Taylor AR, Bizunok NS, McClure-Griffiths NM, Dickey JM, Green AJ (2007) Rotation measures of extragalactic sources behind the southern galactic plane: new insights into the large-scale magnetic field of the inner milky way. Astrophys J 663:258–266. https://doi.org/10.1086/518499, arXiv:0704.0458
Calzetti D, Kennicutt RC (2009) The new frontier: galactic-scale star formation. Publ Astron Soc Pac 121:937–941. https://doi.org/10.1086/605617, 0907.0203
Cameron AGW, Truran JW (1971) The chemical evolution of the galaxy. J Roy Soc Can 65:1
Cartledge SIB, Lauroesch JT, Meyer DM, Sofia UJ (2006) The homogeneity of interstellar elemental abundances in the galactic disk. Astrophys J 641:327–346. https://doi.org/10.1086/500297, astro-ph/0512312
Casagrande L, Schönrich R, Asplund M, Cassisi S, Ramírez I, Meléndez J, Bensby T, Feltzing S (2011) New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey. Astron Astrophys 530:A138. https://doi.org/10.1051/0004-6361/201016276, 1103.4651
Case GL, Bhattacharya D (1998) A new sigma -d relation and its application to the galactic supernova remnant distribution. Astrophys J 504:761, arXiv:astro-ph/9807162
Cerviño M, Knödlseder J, Schaerer D, von Ballmoos P, Meynet G (2000) Gamma-ray line emission from OB associations and young open clusters. I. Evolutionary synthesis models. Astron Astrophys 363:970–983. arXiv:astro-ph/0010283
Chabrier G (2003) Galactic stellar and substellar initial mass function. Publ Astron Soc Pac 115:763–795. https://doi.org/10.1086/376392, astro-ph/0304382
Chabrier G (2005) The initial mass function: from salpeter 1955 to 2005. In: Corbelli E, Palla F, Zinnecker H (eds) The initial mass function 50 years later, astrophysics and space science library, vol 327, p 41. https://doi.org/10.1007/978-1-4020-3407-7_5, astro-ph/0409465
Chabrier G, Hennebelle P, Charlot S (2014) Variations of the stellar initial mass function in the progenitors of massive early-type galaxies and in extreme starburst environments. Astrophys J 796:75. https://doi.org/10.1088/0004-637X/796/2/75, 1409.8466
Chiappini C, Matteucci F, Gratton R (1997) The chemical evolution of the galaxy: the two-infall model. Astrophys J 477:765–780. https://doi.org/10.1086/303726, astro-ph/9609199
Chieffi A, Limongi M (2004) Explosive yields of massive stars from Z = 0 to Z = Z⊙. Astrophys J 608:405–410. https://doi.org/10.1086/392523, arXiv:astro-ph/0402625
Chomiuk L, Povich MS (2011) Toward a unification of star formation rate determinations in the milky way and other galaxies. Astron J 142:197. https://doi.org/10.1088/0004-6256/142/6/197, 1110.4105
Clayton DD (1968) Principles of stellar evolution and nucleosynthesis. McGraw-Hill, New York
Clayton DD (1985) Galactic chemical evolution and nucleocosmochronology: a standard model. In: Arnett WD, Truran JW (eds) Nucleosynthesis: challenges and new developments. University of Chicago Press, Chicago, p 65
Clayton DD (1988) Nuclear cosmochronology within analytic models of the chemical evolution of the solar neighbourhood. Mon Not R Astron Soc 234:1–36. https://doi.org/10.1093/mnras/234.1.1
Cordes JM, Lazio TJW (2002) NE2001.I. A new model for the galactic distribution of free electrons and its fluctuations. ArXiv Astrophysics e-prints. astro-ph/0207156
Cowley C (1995) Introduction to cosmochemistry. Cambridge University Press, Cambridge
Crutcher RM (1999) Magnetic fields in molecular clouds: observations confront theory. Astrophys J 520:706–713. https://doi.org/10.1086/307483
Crutcher RM (2007) Magnetic fields in molecular clouds. EAS Publications Ser 23:37–54. https://doi.org/10.1051/eas:2007004
Dame TM (1993) The distribution of neutral gas in the milky way. In: Holt SS, Verter F (eds) Back to the galaxy. American Institute of Physics conference series, vol 278, pp 267–278
Diehl R, Halloin H, Kretschmer K, Lichti GG, Schönfelder V, Strong AW, von Kienlin A, Wang W, Jean P, Knödlseder J, Roques JP, Weidenspointner G, Schanne S, Hartmann DH, Winkler C, Wunderer C (2006) Radioactive 26al from massive stars in the galaxy. Nature 439:45–47. arXiv:astro-ph/0601015
Edvardsson B, Andersen J, Gustafsson B, Lambert DL, Nissen PE, Tomkin J (1993a) The chemical evolution of the galactic disk - part one - analysis and results. Astron Astrophys 275:101
Edvardsson B, Andersen J, Gustafsson B, Lambert DL, Nissen PE, Tomkin J (1993b) The chemical evolution of the galactic disk - part two - observational data. Astron Astrophys Suppl 102:603
Eggen OJ, Lynden-Bell D, Sandage AR (1962) Evidence from the motions of old stars that the Galaxy collapsed. Astrophys J 136:748. https://doi.org/10.1086/147433
Elmegreen BG (2002) Star formation from large to small scales. Astrophys Space Sci 281:83–95
Englmaier P, Gerhard O (1999) Gas dynamics and large-scale morphology of the Milky Way galaxy. Mon Not R Astron Soc 304:512–534
Feltzing S, Holmberg J, Hurley JR (2001) The solar neighbourhood age-metallicity relation - does it exist? Astron Astrophys 377:911–924. https://doi.org/10.1051/0004-6361:20011119, astro-ph/0108191
Ferriere K (1998) Global model of the interstellar medium in our Galaxy with new constraints on the hot gas component. Astrophys J 497:759. https://doi.org/10.1086/305469
Ferrière KM (2001) The interstellar environment of our galaxy. Rev Mod Phys 73:1031–1066. arXiv:astro-ph/0106359
Ferrière K, Gillard W, Jean P (2007) Spatial distribution of interstellar gas in the innermost 3 kpc of our galaxy. Astron Astrophys 467:611–627. https://doi.org/10.1051/0004-6361:20066992
Figer DF, Rich RM, Kim SS, Morris M, Serabyn E (2004) An extended star formation history for the galactic center from hubble space telescope nicmos observations. Astrophys J 601:319–339. arXiv:astro-ph/0309757
Flynn C, Holmberg J, Portinari L, Fuchs B, Jahreiß H (2006) On the mass-to-light ratio of the local galactic disc and the optical luminosity of the galaxy. Mon Not R Astron Soc 372:1149–1160. arXiv:astro-ph/0608193
François P, Matteucci F, Cayrel R, Spite M, Spite F, Chiappini C (2004) The evolution of the milky way from its earliest phases: constraints on stellar nucleosynthesis. Astron Astrophys 421:613–621. https://doi.org/10.1051/0004-6361:20034140, astro-ph/0401499
Freudenreich HT (1998) A cobe model of the galactic bar and disk. Astrophys J 492:495, arXiv:astro-ph/9707340
Frisch PC, Bzowski M, Grün E, Izmodenov V, Krüger H, Linsky JL, McComas DJ, Möbius E, Redfield S, Schwadron N, Shelton R, Slavin JD, Wood BE (2009) The galactic environment of the sun: interstellar material inside and outside of the heliosphere. Space Sci Rev 146:235–273. https://doi.org/10.1007/s11214-009-9502-0
Fukugita M, Peebles PJE (2004) The cosmic energy inventory. Astrophys J 616:643–668. https://doi.org/10.1086/425155, astro-ph/0406095
Gaidos E, Krot AN, Williams JP, Raymond SN (2009) 26Al and the formation of the solar system from a molecular cloud contaminated by Wolf-Rayet winds. Astrophys J 696:1854–1863. https://doi.org/10.1088/0004-637X/696/2/1854, 0901.3364
Gentile G, Tonini C, Salucci P (2007) Λcdm halo density profiles: where do actual halos converge to nfw ones? Astron Astrophys 467:925–931. arXiv:astro-ph/0701550
Gillessen S, Eisenhauer F, Trippe S, Alexander T, Genzel R, Martins F, Ott T (2008) Monitoring stellar orbits around the massive black hole in the galactic center. ArXiv e-prints 0810.4674
Gilmore G, Reid N (1983) New light on faint stars. iii - galactic structure towards the south pole and the galactic thick disc. Mon Not R Astron Soc 202:1025–1047
Goldsmith PF (1987) Molecular clouds - an overview. In: Hollenbach DJ, Thronson HA Jr (eds) Interstellar processes, astrophysics and space science library, vol 134, pp 51–70
Grand RJJ, Kawata D, Cropper M (2014) Orbits of radial migrators and non-migrators around a spiral arm in N-body simulations. Mon Not R Astron Soc 439:623–638. https://doi.org/10.1093/mnras/stt2483, 1310.2952
Groenewegen MAT, Udalski A, Bono G (2008) The distance to the galactic centre based on population ii cepheids and rr lyrae stars. Astron Astrophys 481:441–448. arXiv:0801.2652
Guibert J, Lequeux J, Viallefond F (1978) Star formation in interstellar gas density in our galaxy. Astron Astrophys 68:1–2
Han JL, Manchester RN, Berkhuijsen EM, Beck R (1997) Antisymmetric rotation measures in our Galaxy: evidence for an A0 dynamo. Astron Astrophys 322:98–102
Han JL, Manchester RN, Qiao GJ (1999) Pulsar rotation measures and the magnetic structure of our Galaxy. Mon Not R Astron Soc 306:371–380. arXiv:astro-ph/9903101
Han JL, Ferriere K, Manchester RN (2004) The spatial energy spectrum of magnetic fields in our Galaxy. Astrophys J 610:820–826. https://doi.org/10.1086/421760, arXiv:astro-ph/0404221
Han JL, Manchester RN, Lyne AG, Qiao GJ, van Straten W (2006) Pulsar rotation measures and the large-scale structure of the galactic magnetic field. Astrophys J 642:868–881. https://doi.org/10.1086/501444, arXiv:astro-ph/0601357
Heckman TM, Armus L, Miley GK (1990) On the nature and implications of starburst-driven galactic superwinds. Astrophys J Suppl 74:833–868. https://doi.org/10.1086/191522
Heiles C (1996) The local direction and curvature of the galactic magnetic field derived from starlight polarization. Astrophys J 462:316. https://doi.org/10.1086/177153
Heiles C, Troland TH (2005) The millennium arecibo 21 centimeter absorption-line survey. IV. Statistics of magnetic field, column density, and turbulence. Astrophys J 624:773–793. https://doi.org/10.1086/428896, arXiv:astro-ph/0501482
Holmberg J, Flynn C (2004) The local surface density of disc matter mapped by Hipparcos. Mon Not R Astron Soc 352:440–446. arXiv:astro-ph/0405155
Holmberg J, Nordström B, Andersen J (2007) The Geneva-Copenhagen survey of the Solar neighbourhood II. New uvby calibrations and rediscussion of stellar ages, the G dwarf problem, age-metallicity diagram, and heating mechanisms of the disk. Astron Astrophys 475:519–537. https://doi.org/10.1051/0004-6361:20077221, 0707.1891
Inoue M, Tabara H (1981) Structure of the galactic magnetic field in the solar neighborhood. Publ Astron Soc Jpn 33:603
Iwamoto K, Brachwitz F, Nomoto K, Kishimoto N, Umeda H, Hix WR, Thielemann FK (1999) Nucleosynthesis in Chandrasekhar mass models for type ia supernovae and constraints on progenitor systems and burning-front propagation. Astrophys J Suppl 125:439–462. arXiv:astro-ph/0002337
Jappsen AK, Klessen RS, Larson RB, Li Y, Mac Low MM (2005) The stellar mass spectrum from non-isothermal gravoturbulent fragmentation. Astron Astrophys 435:611–623. https://doi.org/10.1051/0004-6361:20042178, astro-ph/0410351
Jones A (2009) The role of dust in the interstellar medium: dust sources and dust evolution. In: Pagani L, Gerin M (eds) EAS publications series, vol 34, pp 107–118. https://doi.org/10.1051/eas:0934008
Jurić M, Ivezić Ž, Brooks A, Lupton RH, Schlegel D, Finkbeiner D, Padmanabhan N, Bond N, Sesar B, Rockosi CM, Knapp GR, Gunn JE, Sumi T, Schneider DP, Barentine JC, Brewington HJ, Brinkmann J, Fukugita M, Harvanek M, Kleinman SJ, Krzesinski J, Long D, Neilsen EH Jr, Nitta A, Snedden SA, York DG (2008) The milky way tomography with sdss. i. Stellar number density distribution. Astrophys J 673:864–914
Kalberla PMW, Dedes L (2008) Global properties of the HI distribution in the outer Milky Way. ArXiv e-prints 804. 0804.4831
Kazantzidis S, Kravtsov AV, Zentner AR, Allgood B, Nagai D, Moore B (2004) The effect of gas cooling on the shapes of dark matter halos. Astrophys J 611:L73–L76. https://doi.org/10.1086/423992, astro-ph/0405189
Kennicutt RC Jr (1998) Star formation in Galaxies along the hubble sequence. Annu Rev Astron Astrophys 36:189–232. https://doi.org/10.1146/annurev.astro.36.1.189, arXiv:astro-ph/9807187
Kroupa P (2002) The initial mass function of stars: evidence for uniformity in variable systems. Science 295:82–91. https://doi.org/10.1126/science.1067524, arXiv:astro-ph/0201098
Kroupa P, Weidner C, Pflamm-Altenburg J, Thies I, Dabringhausen J, Marks M, Maschberger T (2013) The stellar and sub-stellar initial mass function of simple and composite populations, p 115. https://doi.org/10.1007/978-94-007-5612-0
Krumholz MR (2014) The big problems in star formation: the star formation rate, stellar clustering, and the initial mass function. Phys Rep 539:49–134. https://doi.org/10.1016/j.physrep.2014.02.001, 1402.0867
Kubryk M, Prantzos N, Athanassoula E (2013) Radial migration in a bar-dominated disc galaxy - I. Impact on chemical evolution. Mon Not R Astron Soc 436:1479–1491. https://doi.org/10.1093/mnras/stt1667
Kubryk M, Prantzos N, Athanassoula E (2015a) Evolution of the Milky Way with radial motions of stars and gas. I. The solar neighbourhood and the thin and thick disks. Astron Astrophys 580:A126. https://doi.org/10.1051/0004-6361/201424171, 1412.0585
Kubryk M, Prantzos N, Athanassoula E (2015b) Evolution of the Milky Way with radial motions of stars and gas. II. The evolution of abundance profiles from H to Ni. Astron Astrophys 580:A127. https://doi.org/10.1051/0004-6361/201424599, 1412.4859
Kulkarni SR, Heiles C (1987) The atomic component. In: Hollenbach DJ, Thronson HA Jr (eds) Interstellar processes. Astrophysics and space science library, vol 134, pp 87–122
Launhardt R, Zylka R, Mezger PG (2002) The nuclear bulge of the galaxy. iii. Large-scale physical characteristics of stars and interstellar matter. Astron Astrophys 384:112–139. arXiv:astro-ph/0201294
Limongi M, Chieffi A (2009) Presupernova evolution and explosion of massive stars: the role of mass loss during the Wolf-Rayet stage. Mem Soc Ast Ital 80:151
Liszt HS, Burton WB (1980) The gas distribution in the central region of the Galaxy. III - A barlike model of the inner-Galaxy gas based on improved HI data. Astrophys J 236:779–797. https://doi.org/10.1086/157803
Lodders K (2003) Solar system abundances and condensation temperatures of the elements. Astrophys J 591:1220–1247. https://doi.org/10.1086/375492
Loebman SR, Roškar R, Debattista VP, Ivezić Ž, Quinn TR, Wadsley J (2011) The genesis of the Milky Way’s thick disk via stellar migration. Astrophys J 737:8. https://doi.org/10.1088/0004-637X/737/1/8, 1009.5997
Lyne AG, Manchester RN, Taylor JH (1985) The galactic population of pulsars. Mon Not R Astron Soc 213:613–639
Maness H, Martins F, Trippe S, Genzel R, Graham JR, Sheehy C, Salaris M, Gillessen S, Alexander T, Paumard T, Ott T, Abuter R, Eisenhauer F (2007) Evidence for a long-standing top-heavy initial mass function in the central parsec of the galaxy. Astrophys J 669:1024–1041. arXiv:0707.2382
Mannucci F, Della Valle M, Panagia N, Cappellaro E, Cresci G, Maiolino R, Petrosian A, Turatto M (2005) The supernova rate per unit mass. Astron Astrophys 433:807–814. https://doi.org/10.1051/0004-6361:20041411, astro-ph/0411450
Maoz D, Graur O (2017) Star formation, supernovae, iron, and α: consistent cosmic and galactic histories. Astrophys J 848:25. https://doi.org/10.3847/1538-4357/aa8b6e, 1703.04540
Matteucci F, Francois P (1989) Galactic chemical evolution - abundance gradients of individual elements. Mon Not R Astron Soc 239:885–904. https://doi.org/10.1093/mnras/239.3.885
McKee CF, Ostriker EC (2007) Theory of star formation. Annu Rev Astron Astrophys 45:565–687. https://doi.org/10.1146/annurev.astro.45.051806.110602, 0707.3514
McKee CF, Williams JP (1997) The luminosity function of ob associations in the galaxy. Astrophys J 476:144
Men H, Ferriere K, Han JL (2008) Observational constraints on models for the interstellar magnetic field in the Galactic disk. ArXiv e-prints 805. 0805.3454
Minchev I, Chiappini C, Martig M (2013) Chemodynamical evolution of the Milky Way disk. I. The solar vicinity. Astron Astrophys 558:A9. https://doi.org/10.1051/0004-6361/201220189, 1208.1506
Minter AH, Spangler SR (1996) Observation of turbulent fluctuations in the interstellar plasma density and magnetic field on spatial scales of 0.01 to 100 parsecs. Astrophys J 458:194. https://doi.org/10.1086/176803
Nakanishi H, Sofue Y (2003) Three-dimensional distribution of the ISM in the Milky Way Galaxy: I. The H I disk. Publ Astron Soc Jpn 55:191–202. arXiv:astro-ph/0304338
Nakanishi H, Sofue Y (2006) Three-dimensional distribution of the ISM in the Milky Way Galaxy: II. The molecular gas disk. Publ Astron Soc Jpn 58:847–860, arXiv:astro-ph/0610769
Navarro JF, Frenk CS, White SDM (1996) The structure of cold dark matter halos. Astrophys J 462:563. https://doi.org/10.1086/177173, astro-ph/9508025
Nomoto K, Tominaga N, Umeda H, Kobayashi C, Maeda K (2006) Nucleosynthesis yields of core-collapse supernovae and hypernovae, and galactic chemical evolution. Nucl Phys A 777:424–458. https://doi.org/10.1016/j.nuclphysa.2006.05.008, arXiv:astro-ph/0605725
Nordström B, Mayor M, Andersen J, Holmberg J, Pont F, Jørgensen BR, Olsen EH, Udry S, Mowlavi N (2004) The Geneva-Copenhagen survey of the solar neighbourhood. ages, metallicities, and kinematic properties of 14 000 f and g dwarfs. Astron Astrophys 418:989–1019, arXiv:astro-ph/0405198
Oey MS, Meurer GR, Yelda S, Furst EJ, Caballero-Nieves SM, Hanish DJ, Levesque EM, Thilker DA, Walth GL, Bland-Hawthorn J, Dopita MA, Ferguson HC, Heckman TM, Doyle MT, Drinkwater MJ, Freeman KC, Kennicutt RC Jr, Kilborn VA, Knezek PM, Koribalski B, Meyer M, Putman ME, Ryan-Weber EV, Smith RC, Staveley-Smith L, Webster RL, Werk J, Zwaan MA (2007) The survey for ionization in neutral gas Galaxies. III. Diffuse, warm ionized medium and escape of ionizing radiation. Astrophys J 661:801–814. https://doi.org/10.1086/517867, arXiv:astro-ph/0703033
Olling RP, Merrifield MR (2001) Luminous and dark matter in the Milky Way. Mon Not R Astron Soc 326:164–180. https://doi.org/10.1046/j.1365-8711.2001.04581.x, arXiv:astro-ph/0104465
Pagel BEJ (1997) Nucleosynthesis and chemical evolution of Galaxies. Cambridge University Press, Cambridge
Pejcha O, Prieto JL (2015) On the intrinsic diversity of type II-plateau supernovae. Astrophys J 806:225. https://doi.org/10.1088/0004-637X/806/2/225, 1501.06573
Pettini M (2004) Element abundances through the cosmic ages. In: Esteban C, García López R, Herrero A, Sánchez F (eds) Cosmochemistry. The melting pot of the elements, pp 257–298, astro-ph/0303272
Pfalzner S (2009) Universality of young cluster sequences. Astron Astrophys 498:L37–L40. https://doi.org/10.1051/0004-6361/200912056, 0904.0523
Pohl M, Englmaier P, Bissantz N (2008) Three-dimensional distribution of molecular gas in the barred Milky Way. Astrophys J 677:283–291. https://doi.org/10.1086/529004, arXiv:0712.4264
Prantzos N, Boissier S (2010) The SNIa/CCSN ratio as a function of metallicity. In: Progenitors and Environments of Stellar Explosions, p 77
Prantzos N, Silk J (1998) Star formation and chemical evolution in the Milky Way: cosmological implications. Astrophys J 507:229–240. https://doi.org/10.1086/306327
Prantzos N, Boehm C, Bykov AM, Diehl R, Ferrière K, Guessoum N, Jean P, Knoedlseder J, Marcowith A, Moskalenko IV, Strong A, Weidenspointner G (2011) The 511 keV emission from positron annihilation in the Galaxy. Rev Mod Phys 83:1001–1056. https://doi.org/10.1103/RevModPhys.83.1001, 1009.4620
Plüeschke S, Diehl R, Schöenfelder V, Bloemen H, Hermsen W, Bennett K, Winkler C, McConnell M, Ryan J, Oberlack U, Knöedlseder J (2001) In: Gimenez A, Reglero V, Winkler C (eds) Exploring the gamma-ray universe. ESA Special Publication, vol 459
Rand RJ, Kulkarni SR (1989) The local Galactic magnetic field. Astrophys J 343:760–772. https://doi.org/10.1086/167747
Rand RJ, Lyne AG (1994) New rotation measures of distant pulsars in the inner galaxy and magnetic field reversals. Mon Not R Astron Soc 268:497
Rattenbury NJ, Mao S, Sumi T, Smith MC (2007) Modelling the galactic bar using ogle-ii red clump giant stars. Mon Not R Astron Soc 378:1064–1078. arXiv:0704.1614
Robin AC, Reylé C, Derrière S, Picaud S (2003) A synthetic view on structure and evolution of the milky way. Astron Astrophys 409:523–540. arXiv:astro-ph/0401052
Rocha-Pinto HJ, Maciel WJ, Scalo J, Flynn C (2000) Chemical enrichment and star formation in the Milky Way disk. I. Sample description and chromospheric age-metallicity relation. Astron Astrophys 358:850–868. astro-ph/0001382
Roškar R, Debattista VP, Quinn TR, Stinson GS, Wadsley J (2008) Riding the spiral waves: implications of stellar migration for the properties of galactic disks. Astrophys J 684:L79. https://doi.org/10.1086/592231, 0808.0206
Russeil D (2003) Star-forming complexes and the spiral structure of our Galaxy. Astron Astrophys 397:133–146. https://doi.org/10.1051/0004-6361:20021504
Russeil D (2010) The disk of our Galaxy. High Astron 15:786–786. https://doi.org/10.1017/S1743921310011646
Salpeter EE (1955) The luminosity function and stellar evolution. Astrophys J 121:161. https://doi.org/10.1086/145971
Sawada T, Hasegawa T, Handa T, Cohen RJ (2004) A molecular face-on view of the galactic centre region. Mon Not R Astron Soc 349:1167–1178. https://doi.org/10.1111/j.1365-2966.2004.07603.x, arXiv:astro-ph/0401286
Scalo JM (1986) The initial mass function of massive stars in galaxies empirical evidence. In: de Loore CWH, Willis AJ, Laskarides P (eds) Luminous stars and associations in Galaxies, IAU Symposium, vol 116, pp 451–466
Schaller G, Schaerer D, Meynet G, Maeder (1992) A new grids of stellar models from 0.8 to 120 solar masses at Z = 0.020 and Z = 0.001. Astron Astrophys Suppl Ser 96:269–331
Schmidt M (1959) The rate of star formation. Astrophys J 129:243. https://doi.org/10.1086/146614
Schmidt M (1963) The rate of star formation. II. The rate of formation of stars of different mass. Astrophys J 137:758. https://doi.org/10.1086/147553
Schönrich R, Binney J (2009) Origin and structure of the Galactic disc(s). Mon Not R Astron Soc 399:1145–1156. https://doi.org/10.1111/j.1365-2966.2009.15365.x, 0907.1899
Sedlmayr E, Patzer ABC (2004) Grain formation and dynamical atmosphere. In: A Jorissen, S Goriely, M Rayet, L Siess, H Boffin (eds) EAS publications series, vol 11, pp 51–66. https://doi.org/10.1051/eas:2004003
Sellwood JA, Binney JJ (2002) Radial mixing in galactic discs. Mon Not R Astron Soc 336:785–796. https://doi.org/10.1046/j.1365-8711.2002.05806.x, astro-ph/0203510
Sofue Y, Honma M, Omodaka T (2008) Unified rotation curve of the galaxy—decomposition into de Vaucouleurs bulge, disk, dark halo, and the 9-kpc rotation dip –. ArXiv e-prints 0811.0859
Sommer-Larsen J, Dolgov A (2001) Formation of disk galaxies: warm dark matter and the angular momentum problem. Astrophys J 551:608–623. https://doi.org/10.1086/320211, astro-ph/9912166
Soubiran C, Girard P (2005) Abundance trends in kinematical groups of the Milky Way’s disk. Astron Astrophys 438:139–151. https://doi.org/10.1051/0004-6361:20042390, astro-ph/0503498
Spano M, Marcelin M, Amram P, Carignan C, Epinat B, Hernandez O (2008) Ghasp: an hα kinematic survey of spiral and irregular galaxies - v. Dark matter distribution in 36 nearby spiral galaxies. Mon Not R Astron Soc 383:297–316. 0710.1345
Springel V, White SDM, Frenk CS, Navarro JF, Jenkins A, Vogelsberger M, Wang J, Ludlow A, Helmi A (2008) Prospects for detecting supersymmetric dark matter in the galactic halo. Nature 456:73–76, 0809.0894
Sukhbold T, Ertl T, Woosley SE, Brown JM, Janka HT (2016) Core-collapse Supernovae from 9 to 120 solar masses based on neutrino-powered explosions. Astrophys J 821:38. https://doi.org/10.3847/0004-637X/821/1/38, 1510.04643
Tammann GA, Loeffler W, Schroeder A (1994) The galactic supernova rate. Astrophys J Suppl 92:487–493
Thorsett SE, Chakrabarty D (1999) Neutron star mass measurements. I. Radio pulsars. Astrophys J 512:288–299. https://doi.org/10.1086/306742, astro-ph/9803260
Tinsley BM (1980) Evolution of the stars and gas in Galaxies. Fundam Cosm Phys 5:287–388
Troland TH, Heiles C (1986) Interstellar magnetic field strengths and gas densities observational and theoretical perspectives. Astrophys J 301:339–345. https://doi.org/10.1086/163904
Truran JW, Cameron AGW (1971) Evolutionary models of nucleosynthesis in the Galaxy. Astrophys Space Sci 14:179–222. https://doi.org/10.1007/BF00649203
Vallée JP (2005) Pulsar-based galactic magnetic map: a large-scale clockwise magnetic field with an anticlockwise annulus. Astrophys J 619:297–305. https://doi.org/10.1086/426182
Vallée JP (2017) A guided map to the spiral arms in the galactic disk of the Milky Way. Astron Rev 13:113–146. https://doi.org/10.1080/21672857.2017.1379459, 1711.05228
Vázquez-Semadeni E (2015) Interstellar MHD turbulence and star formation. In: Lazarian A, de Gouveia Dal Pino EM, Melioli C (eds) Magnetic fields in diffuse media, astrophysics and space science library, vol 407, p 401. https://doi.org/10.1007/978-3-662-44625-6-14, 1208.4132
Villalobos Á, Helmi A (2008) Simulations of minor mergers - I. General properties of thick discs. Mon Not R Astron Soc 391:1806–1827. https://doi.org/10.1111/j.1365-2966.2008.13979.x
Voss R, Diehl R, Hartmann DH, Cerviño M, Vink JS, Meynet G, Limongi M, Chieffi A (2009) Using population synthesis of massive stars to study the interstellar medium near OB associations. Astron Astrophys 504:531–542. https://doi.org/10.1051/0004-6361/200912260, 0907.5209
Wang B (2018) Mass-accreting white dwarfs and type Ia supernovae. ArXiv e-prints 1801.04031
Weidemann V (2000) Revision of the initial-to-final mass relation. Astron Astrophys 363:647–656
Weidner C, Kroupa P, Bonnell IAD (2010) The relation between the most-massive star and its parental star cluster mass. Mon Not R Astron Soc 401:275–293. https://doi.org/10.1111/j.1365-2966.2009.15633.x, 0909.1555
Weidner C, Pflamm-Altenburg J, Kroupa P (2011) The Galaxy-wide IMF - from Star Clusters to Galaxies. In: Treyer M, Wyder T, Neill J, Seibert M, Lee J (eds) UP2010: have observations revealed a variable upper end of the initial mass function? Astronomical Society of the Pacific conference series, vol 440, p 19. 1011.1905
Weidner C, Kroupa P, Pflamm-Altenburg J (2013) The mmax-Mecl relation, the IMF and IGIMF: probabilistically sampled functions. Mon Not R Astron Soc 434:84–101. https://doi.org/10.1093/mnras/stt1002, 1306.1229
Woosley SE, Heger A (2007) Nucleosynthesis and remnants in massive stars of solar metallicity. Phys Rep 442:269–283. https://doi.org/10.1016/j.physrep.2007.02.009, arXiv:astro-ph/0702176
Woosley SE, Weaver TA (1995) The evolution and explosion of massive stars. II. Explosive hydrodynamics and nucleosynthesis. Astrophys J Suppl 101:181. https://doi.org/10.1086/192237
Zinnecker H, Yorke HW (2007) Toward understanding massive star formation. Annu Rev Astron Astrophys 45:481–563. https://doi.org/10.1146/annurev.astro.44.051905.092549, 0707.1279
Zoccali M, Renzini A, Ortolani S, Greggio L, Saviane I, Cassisi S, Rejkuba M, Barbuy B, Rich RM, Bica E (2003) Age and metallicity distribution of the galactic bulge from extensive optical and near-ir stellar photometry. Astron Astrophys 399:931–956. arXiv:astro-ph/0210660
Zuckerman B, Evans NJ II (1974) Models of massive molecular clouds. Astrophys J 192:L149–L152. https://doi.org/10.1086/181613
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Diehl, R., Prantzos, N. (2018). Cosmic Evolution of Isotopic Abundances: Basics. In: Diehl, R., Hartmann, D., Prantzos, N. (eds) Astrophysics with Radioactive Isotopes. Astrophysics and Space Science Library, vol 453. Springer, Cham. https://doi.org/10.1007/978-3-319-91929-4_11
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