Abstract
This chapter presents a description of the interstellar medium. It starts with a summary of the interstellar medium structure and how the various phases are related to each other. The emphasis is put on molecular clouds, and on their densest regions, the dense cores, which are the birth place of stars. The evolution of matter during the star formation process and its observable consequences, especially in term of chemical composition is presented. The next section is dedicated to the constituents of the interstellar medium, with separate presentations of the gas species and the dust grains. Methods used by astronomers to derive useful information on the structure, temperature, ionization rate of interstellar environments as well as magnetic fields are briefly described. The last part of the chapter presents the telescopes and their instruments used for studying the interstellar medium across the electromagnetic spectrum.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Notes
- 1.
It is customary to quote interstellar pressures as the product of the temperature and particle density, since the equation of state of ideal gas applies to these very dilute media (PV = nRT).
References
Bertoldi F, Cox P, Neri R et al (2003) High-excitation CO in a quasar host galaxy at z = 6.42. Astron Astrophys 409:47
Noterdaeme P, Petitjean P, Srianand R, Ledoux C, López S (2011) The evolution of the cosmic microwave background temperature. Measurements of TCMB at high redshift from carbon monoxide excitation. Astron Astrophys 526:L7
Draine B (2011) Physics of the interstellar and intergalactic medium, Princeton series in astrophysics. Princeton University Press, Princeton
Ostriker EC, McKee CF, Leroy AK (2010) Regulation of star formation rates in multiphase galactic disks: a thermal/dynamical equilibrium model. Astrophys J 721:975
Wood KH, Alex S, Joung MR, Mac Low MM, Benjamin RA, Haffner LM, Reynolds RJ, Madsen GJ (2010) Photoionization of high-altitude gas in a Supernova-driven turbulent interstellar medium. Astrophys J 721:1397
Field GB, Goldsmith DW, Habing HJ (1969) Cosmic-ray heating of the interstellar gas. Astrophys J 155:L149
Jenkins EB, Tripp TM (2011) The distribution of thermal pressures in the diffuse, cold neutral medium of our galaxy. II. An expanded survey of interstellar C I fine-structure excitations. Astrophys J 734:65
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
Audit E, Hennebelle P (2010) On the structure of the turbulent interstellar clouds. Influence of the equation of state on the dynamics of 3D compressible flows. Astron Astrophys 511:A76
Rachford BL, Snow TP, Destree JD et al (2009) Molecular hydrogen in the far ultraviolet spectroscopic explorer translucent lines of sight: the full sample. Astrophys J Suppl 180:125
Miville-Deschênes M-A, Martin PG, Abergel A et al (2010) Herschel-SPIRE observations of the Polaris flare: structure of the diffuse interstellar medium at the sub-parsec scale. Astron Astrophys 518:L10
Roman-Duval J, Jackson JM, Heyer M, Rathborne J, Simon R (2010) Physical properties and galactic distribution of molecular clouds identified in the galactic ring survey. Astrophys J 723:492
Kolmogorov A (1941) The local structure of turbulence in incompressible viscous fluid for very large Reynolds’ numbers. DoSSR 30:301
Falgarone E, Hily-Blant P, Pety J (2009) Intermittency of interstellar turbulence: extreme velocity-shears and CO emission on milliparsec scale. Astron Astrophys 507:355; Lis DC, Vaillancourt JE, Goldsmith PF, Bell TA, Scoville NZ, Zmuidzinas J (eds) (2009) Submillimeter astrophysics and technology: a symposium honoring Thomas G. Phillips. ASP conference series, vol 417. Astronomical Society of the Pacific, San Francisco, p 243
Lada CJ, Lombardi M, Alves J (2010) On the star formation rates in molecular clouds. Astrophys J 724:687
André P et al (2010) From filamentary clouds to prestellar cores to the stellar IMF: initial highlights from the Herschel Gould Belt Survey. Astron Astrophys 518:L102
Alves JF, Lada CJ, Lada EA (2001) Internal structure of a cold dark molecular cloud inferred from the extinction of background starlight. Nature 409:159
Caselli P, van der Tak FFS, Ceccarelli C, Bacmann A (2003) Abundant H2D+ in the pre-stellar core L1544. Astron Astrophys 403:L37
Pérault M, Omont A, Simon G (1996) First ISOCAM images of the Milky Way. Astron Astrophys 315:L165
Peretto N, Fuller GA (2010) A statistical study of the mass and density structure of infrared dark clouds. Astrophys J 723:555
Herbst E, van Dishoeck E (2009) Complex organic interstellar molecules. Annu Rev Astron Astrophys 47:427
Parise B, Castets A, Herbst E, Caux E, Ceccarelli C, Mukhopadhyay I, Tielens AGGM (2004) First detection of triply-deuterated methanol. Astron Astrophys 416:159
Stark R, Sandell G, Beck SC et al (2004) Probing the early stages of low-mass star formation in LDN 1689Â N: dust and water in IRAS 16293-2422A, B, and E. Astrophys J 608:341
Commerçon B, Hennebelle P, Audit E, Chabrier G, Teyssier R (2010) Protostellar collapse: radiative and magnetic feedbacks on small-scale fragmentation. Astron Astrophys 510:L3
Mouschovias T, Spitzer L (1976) Note on the collapse of magnetic interstellar clouds. Astrophys J 210:326
Bergin E, Tafalla M (2007) Cold dark clouds: the initial conditions for star formation. Annu Rev Astron Astrophys 45:339
Pety J, Gueth F, Guilloteau S, Dutrey A (2006) Plateau de Bure interferometer observations of the disk and outflow of HH 30. Astron Astrophys 458:841
Burrows CJ, Stapelfeldt KR, Watson AM (1996) Hubble space telescope observations of the disk and jet of HH 30. Astrophys J 473:437
Levinson HF, Morbidelli A, Tsiganis K, Nesvorný D, Gomes R (2011) Late orbital instabilities in the outer planets induced by interaction with a self-gravitating planetesimal disk. Astron J 142:152
Lagrange AM, Bonnefoy M, Chauvin G et al (2010) A giant planet imaged in the disk of the young star β Pictoris. Science 329:57
Gerin M, Pety J, Goicoechea JR (2009) The horsehead nebula, a template source for interstellar physics and chemistry. In: Lis DC, Vaillancourt JE, Goldsmith PF, Bell TA, Scoville NZ, Zmuidzinas J (eds) Submillimeter astrophysics and technology: a symposium honoring Thomas G. Phillips. ASP conference series, vol 417. Astronomical Society of the Pacific, San Francisco, p 165
Gonzalez GM, Le Bourlot J, le Petit F, Roueff E (2008) Radiative transfer revisited for emission lines in photon dominated regions. Astron Astrophys 485:127
Glover SCO, Federrath C, Mac Low MM, Klessen RS (2010) Modelling CO formation in the turbulent interstellar medium. Mon Notices R Astron Soc 404:2
Draine BT, Mc Kee CF (1993) Theory of interstellar shocks. Annu Rev Astron Astrophys 31:373
Nisini B, Benedettini M, Codella C et al (2010) Water cooling of shocks in protostellar outflows: Herschel-PACS map of L1157. Astron Astrophys 518:L120
Troscompt N, Faure A, Wiesenfeld L, Ceccarelli C, Valiron P (2009) Rotational excitation of formaldehyde by hydrogen molecules: ortho-H2CO at low temperature. Astron Astrophys 493:687
Maret S, Faure A, Scifoni E, Wiesenfeld L (2009) On the robustness of the ammonia thermometer. Mon Notices R Astron Soc 399:425
van der Tak FFS, Black JH, Schöier FL, Jansen DJ, van Dishoeck EF (2007) A computer program for fast non-LTE analysis of interstellar line spectra with diagnostic plots to interpret observed line intensity ratios. Astron Astrophys 468:627
Goicoechea JR, Pety J, Gerin M, Hily-Blant P, Le Bourlot J (2009) The ionization fraction gradient across the Horsehead edge: an archetype for molecular clouds. Astron Astrophys 498:771
Indriolo N, McCall BJ (2012) Investigating the cosmic-ray ionization rate in the galactic diffuse interstellar medium through observations of H +3 . Astrophys J 745:91
Neufeld D, Goicoechea JR, Sonnentrucker P et al (2010) Herschel/HIFI observations of interstellar OH+ and H2O+ towards W49N: a probe of diffuse clouds with a small molecular fraction. Astron Astrophys 521:L10
Crutcher RM (2009) OH and CN Zeeman observations of magnetic fields in molecular clouds. Rev Mex de Astron y Astrofisica (Serie de Conferencias) 36:107
Godard B, Falgarone E, Pineau Des Forets G (2009) Models of turbulent dissipation regions in the diffuse interstellar medium. Astron Astrophys 495:847
Gibb EL, Whittet DCB, Boogert ACA, Tielens AGGM (2004) Interstellar ice: the infrared space observatory legacy. Astrophys J 151:35
Motte F, Zavagno A, Bontemps S et al (2010) Initial highlights of the HOBYS key program, the Herschel imaging survey of OB young stellar objects. Astron Astrophys 518:L77
Joblin C, Tielens AGGM (eds) (2011) PAHs and the universe: a symposium to celebrate the 25th anniversary of the PAH hypothesis. EAS publications series, vol 46. EDP Sciences, Les Ulis
Jura M (1974) Formation and destruction rates of interstellar H2. Astrophys J 191:375
Le Bourlot J, Le Petit F, Pinto C, Roueff E, Roy F (2012) Surface chemistry in the interstellar medium – I – H2 formation by Langmuir-Hinshelwood and Eley-Rideal mechanisms. Astron Astrophys 541:A76
Danger G, Bossa J-B, de Marcellus P, Borget F, Duvernay F, Theulé P, Chiavassa T, D’Hendecourt L (2011) Experimental investigation of nitrile formation from VUV photochemistry of interstellar ices analogs: acetonitrile and amino acetonitrile. Astron Astrophys 525:30
de Marcellus P, Bertrand M, Nuevo M, Westall F, Le Sergeant d’Hendecourt L (2011) Prebiotic significance of extraterrestrial ice photochemistry: detection of hydantoin in organic residues. Astrobiology 11:847
Lombardi M, Alves J, Lada CJ (2011) 2MASS wide field extinction maps. IV. The Orion, Monoceros R2, Rosette, and Canis Major star forming regions. Astron Astrophys 535:A16
Skrutskie MF, Cutri RM, Stiening R et al (2006) The two micron all sky survey (2MASS). Astron J 131:1163
Pagani L, Steinacker J, Bacmann A, Stutz A, Henning T (2010) The ubiquity of micrometer-sized dust grains in the dense interstellar medium. Science 329:1622
Planck Collaboration, Abergel A, Ade PAR, Aghanim N et al (2011) Planck early results. XXIV. Dust in the diffuse interstellar medium and the galactic halo. Astron Astrophys 536:24
Compiègne M, Verstraete L, Jones A, Bernard J-P, Boulanger F, Flagey N, Le Bourlot J, Paradis D, Ysard N (2011) The global dust SED: tracing the nature and evolution of dust with DustEM. Astron Astrophys 525:A103
Whittet DCB, Hough JH, Lazarian A, Hoang T (2008) The efficiency of grain alignment in dense interstellar clouds: a reassessment of constraints from near-infrared polarization. Astrophys J 764:304
Bergin E, Phillips TG, Comito C et al (2010) Herschel observations of EXtra-Ordinary Sources (HEXOS): the present and future of spectral surveys with Herschel/HIFI. Astron Astrophys 521:L20
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2013 Springer-Verlag Berlin Heidelberg
About this chapter
Cite this chapter
Gerin, M. (2013). The Molecular Universe. In: Smith, I., Cockell, C., Leach, S. (eds) Astrochemistry and Astrobiology. Physical Chemistry in Action. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-31730-9_2
Download citation
DOI: https://doi.org/10.1007/978-3-642-31730-9_2
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-31729-3
Online ISBN: 978-3-642-31730-9
eBook Packages: Chemistry and Materials ScienceChemistry and Material Science (R0)