Abstract
Over the past decade, gamma-ray observations of supernova remnants with space-based instruments, such as Astro-rivelatore Gamma a Immagini LEggero (AGILE) and the Fermi-Large Area Telescope (LAT), and ground-based instruments such as the High Energy Stereoscopic System (H.E.S.S.), the Major Atmospheric Gamma-Ray Imaging Cherenkov (MAGIC) telescopes, and the Very Energetic Radiation Imaging Telescope Array System (VERITAS) have significantly advanced our understanding of particle acceleration in the shocks of these highly energetic objects. The number of supernova remnants (SNRs) that are detected in high-energy light has steadily increased - a clear demonstration that shocks are capable of accelerating particles to multi-TeV energies. While the ultimate proof of SNRs as the dominant source of cosmic rays in our Galaxy is still elusive, uncontroversial evidence points to the acceleration of protons in supernova remnant shells. This chapter aims to review the most important results in the gamma-ray study of supernova remnants.
This is a preview of subscription content, log in via an institution.
References
Abdo AA et al (2010) Fermi-lat discovery of GeV gamma-ray emission from the young supernova remnant cassiopeia A. ApJL 710:L92-L97. doi:10.1088/2041-8205/710/1/L92
Abdo AA et al (2011) Observations of the young supernova remnant RX J1713.7-3946 with the fermi large area telescope. ApJ 734:28. doi:10.1088/0004-637X/734/1/28
Abdo AA et al (2010) Fermi large area telescope observations of the supernova remnant w28 (g6.4-0.1). Astrophys J 718(1):348. arXiv:http://stacks.iop.org/0004-637X/718/i=1/a=348
Abdo AA et al (2009) Fermi LAT discovery of extended gamma-ray emission in the direction of supernova remnant W51C. ApJL 706:L1-L6. doi:10.1088/0004-637X/706/1/L1
Abeysekara AU et al (2013) Sensitivity of the high altitude water Cherenkov detector to sources of multi-TeV gamma rays. Astropart Phys 50:26-32. doi:10.1016/j.astropartphys.2013.08.002
Acciari VA et al (2009) Observation of extended very high energy emission from the supernova remnant IC 443 with VERITAS. ApJL 698:L133-L137. doi:10.1088/0004-637X/698/2/L133
Acciari VA et al (2011) Discovery of TeV gamma-ray emission from Tycho’s supernova remnant. ApJL 730:L20. doi:10.1088/2041-8205/730/2/L20
Acero F et al (2015) The 1st fermi lat supernova remnant catalog. ArXiv e-prints
Acero F et al (2010) H.E.S.S. Collaboration: First detection of VHE γ-rays from SN 1006 by HESS. AAP 516:A62. doi:10.1051/0004-6361/200913916
Acero F et al (2009) A joint spectro-imaging analysis of the XMM-Newton and HESS observations of the supernova remnant RX J1713.7-3946. AAP 505:157-167
Acharya BS et al (2015) The Cherenkov Telescope Array potential for the study of young supernova remnants. Astropart Phys 62:152-164. doi:10.1016/j.astropartphys.2014.08.005
Ackermann M et al (2013) Detection of the characteristic pion-decay signature in supernova remnants. Science 339:807-811. doi:10.1126/science.1231160
Aharonian F et al (2001) Evidence for TeV gamma ray emission from Cassiopeia A. Astron Astrophys 370:112-120
Aharonian F et al (2008) Discovery of very high energy gamma-ray emission coincident with molecular clouds in the W 28 (G6.4-0.1) field. AAP 481:401-410. doi:10.1051/0004-6361:20077765
Aharonian F et al (2006) The H.E.S.S. survey of the inner galaxy in very high energy gamma rays. Astrophys J 636:777-797
Aharonian F et al (2007) Primary particle acceleration above 100 TeV in the shell-type supernova remnant ¡ASTROBJ¿RX J1713.7-3946¡/ASTROBJ¿ with deep HESS observations. Astron Astrophys 464:235-243
Aharonian F et al (2007) H.E.S.S. Observations of the Supernova Remnant RX J0852.0-4622: Shell-type morphology and spectrum of a widely extended very high energy gamma-ray source. Astrophys J 661:236-249
Aharonian F et al (2009) Discovery of gamma-ray emission from the shell-type supernova remnant RCW 86 With Hess. ApJ 692:1500-1505
Aharonian FA (2004)Very High Energy Cosmic Gamma Radiation: A crucial window on the extreme universe. EBSCO ebook academic collection. World Scientific, River Edge
Aharonian FA (2013) Gamma rays from supernova remnants. Astropart Phys 43, 71-80. doi:10.1016/j.astropartphys.2012.08.007
Albert J et al (2007) Observation of VHE γ-rays from Cassiopeia A with the MAGIC telescope. Astron Astrophys 474:937-940
Albert J et al (2007) Discovery of very high energy gamma radiation from IC 443 with the MAGIC telescope. Astrophys J Lett 664:L87-L90 (2007)
Araya M, Frutos F (2012) On the nature of the TeV emission from the supernova remnant SN 1006. MNRAS 425:2810-2816. doi:10.1111/j.1365-2966.2012.21580.x
Bell AR (2004) Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays. MNRAS 353:550-558. doi:10.1111/j.1365-2966.2004.08097.x
Berezhko EG, Ksenofontov LT, Völk HJ (2013) The nature of gamma-ray emission of Tycho’s supernova remnant. ApJ 763:14. doi:10.1088/0004-637X/763/1/14
Blasi P (2013) The origin of galactic cosmic rays. AAPr 21:70. doi:10.1007/s00159-013-0070-7
Blasi P (2014) Recent results in cosmic ray physics and their interpretation. Braz J Phys 44:426-440. doi:10.1007/s13538-014-0223-9
Caprioli D (2012) Cosmic-ray acceleration in supernova remnants: non-linear theory revised. JCAP 7:038. doi:10.1088/1475-7516/2012/07/038
Caragiulo M, Di Venere L (2014) Evidence of hadronic interaction in Tycho supernova remnant using fermi-LAT data. Nucl Phys B Proc Suppl 256:89-93. doi:10.1016/j.nuclphysbps.2014.10.010
Castro D, Slane P (2010) Fermi large area telescope observations of supernova remnants interacting with molecular clouds. ApJ 717:372-378. doi:10.1088/0004-637X/717/1/372
Ellison DC, Vladimirov A (2008) Magnetic field amplification and rapid time variations in SNR RX J1713.7-3946. ApJL 673:L47-L50
Esposito JA, Hunter SD, Kanbach G, Sreekumar, P (1996) EGRET observations of radio-bright supernova remnants. ApJ 461:820-+
Funk, S (2015) Ground- and space-based gamma-ray astronomy. Annu Rev Nucl Part Sci 65(1):245-277. doi 10.1146/annurev-nucl-102014-022036. arXiv:http://dx.doi.org/10.1146/annurev-nucl-102014-022036
Gabici S, Aharonian FA (2014) Hadronic gamma-rays from RX J1713.7-3946? MNRAS 445:L70-L73. doi:10.1093/mnrasl/slu132
Gabici S, Aharonian FA, Casanova S (2009) Broad-band non-thermal emission from molecular clouds illuminated by cosmic rays from nearby supernova remnants. MNRAS 396:1629-1639. doi:10.1111/j.1365-2966.2009.14832.x
Ginzburg VL, Syrovatskii SI (1964) The origin of cosmic rays. The Origin of Cosmic Rays, Macmillan, New York
Giordano F et al (2012) Fermi large area telescope detection of the young supernova remnant Tycho. ApJL 744:L2. doi:10.1088/2041-8205/744/1/L2
Giuliani A et al (2011) Neutral pion emission from accelerated protons in the supernova remnant W44. ApJL 742:L30. doi:10.1088/2041-8205/742/2/L30
H.E.S.S. Collaboration et al (2015) H.E.S.S. reveals a lack of TeV emission from the supernova remnant Puppis A. AAP 575:A81. doi:10.1051/0004-6361/201424805
H.E.S.S. Collaboration et al (2016) Detailed spectral and morphological analysis of the shell type SNR RCW 86. ArXiv e-prints
Hanabata Y et al (2014) Detailed investigation of the gamma-ray emission in the vicinity of snr w28 with fermi-lat. Astrophys J 786(2):145. http://stacks.iop.org/0004-637X/786/i=2/a=145
Hartman RC et al (1999) The third EGRET catalog of high-energy gamma-ray sources. ApJs 123:79-202
H.E.S.S. Collaboration et al (2011) A new SNR with TeV shell-type morphology: HESS J1731-347. AAP 531:A81. doi:10.1051/0004-6361/201016425
Hewitt JW, Grondin MH, Lemoine-Goumard, M., Reposeur T, Ballet J, Tanaka T (2012) Fermi-LAT and WMAP observations of the puppis A supernova remnant. ApJ 759:89. doi:10.1088/0004-637X/759/2/89
Humensky B (2015) for the VERITAS Collaboration: The TeV morphology of the interacting supernova remnant IC 443. ArXiv e-prints
Humensky TB (2008) VERITAS studies of the supernova remnants Cas A and IC 443. In: Aharonian FA, Hofmann W, Rieger F (ed) American Institute of Physics Conference Series, vol. 1085, pp. 357-360
Indebetouw R et al (2014) Dust production and particle acceleration in supernova 1987A revealed with ALMA. ApJL 782:L2. doi:10.1088/2041-8205/782/1/L2
Jogler T, Funk S (2016) Revealing W51C as a cosmic ray source using fermi-LAT data. ApJ 816:100. doi:10.3847/0004-637X/816/2/100
Katsuda S et al (2015) Evidence for thermal X-ray line emission from the synchrotron-dominated supernova remnant RX J1713.7-3946. ApJ 814:29. doi:10.1088/0004-637X/814/1/29
Malkov MA, Diamond PH, Sagdeev RZ (2011) Mechanism for spectral break in cosmic ray proton spectrum of supernova remnant W44. Nat Commun 2:94. doi:10.1038/ncomms1195
Morlino G, Caprioli D (2012) Strong evidence for hadron acceleration in Tycho’s supernova remnant. AAP 538:A81. doi:10.1051/0004-6361/201117855
Renaud M et al (2012) Fermi/LAT Collaboration: Constraints on cosmic-ray efficiency in the supernova remnant RCW 86. In: Aharonian FA, Hofmann W, Rieger FM (eds) American Institute of Physics Conference Series, vol. 1505, pp. 229-232. doi:10.1063/1.4772239
Romero GE, Benaglia P, Torres, DF (1999) Unidentified 3EG gamma-ray sources at low galactic latitudes. AAP 348:868-876
Tanaka T et al (2011) Gamma-ray observations of the supernova remnant RX J0852.0-4622 with the fermi large area telescope. ApJL 740:L51. doi:10.1088/2041-8205/740/2/L51
Tanaka T et al (2008) Study of nonthermal emission from SNR RX J1713.7-3946 with Suzaku. ApJ 685:988-1004
Torres DF, Marrero AYR, de Cea Del Pozo E (2010) The GeV to TeV connection in the environment of SNR IC 443. MNRAS 408:1257-1266. doi:10.1111/j.1365-2966.2010.17205.x
Torres DF, Romero GE, Dame TM, Combi JA, Butt YM (2003) Supernova remnants and γ-ray sources. Phys Rep 382:303-380
Uchiyama Y, Aharonian FA (2008) Fast variability of nonthermal x-ray emission in cassiopeia a: Probing electron acceleration in reverse-shocked ejecta. Astrophys J 677:L105
Uchiyama Y, Aharonian FA, Takahashi T (2003) Fine-structure in the nonthermal X-ray emission of SNR RX J1713.7-3946 revealed by Chandra. Astron Astrophys 400:567-574
Uchiyama Y, Blandford RD, Funk S, Tajima H, Tanaka T (2010) Gamma-ray emission from crushed clouds in supernova remnants. ApJL 723:L122-L126. doi:10.1088/2041-8205/723/1/L122
Uchiyama Y et al (2012) Fermi large area telescope discovery of GeV gamma-ray emission from the vicinity of SNR W44. ApJL 749:L35. doi:10.1088/2041-8205/749/2/L35
Yuan Y, Funk S, Jóhannesson G, Lande J, Tibaldo L, Uchiyama Y (2013) Fermi large area telescope detection of a break in the gamma-ray spectrum of the supernova remnant Cassiopeia A. ApJ 779:117. doi:10.1088/0004-637X/779/2/117
Zirakashvili VN, Aharonian FA (2010)Nonthermal radiation of young supernova remnants: the case of RX J1713.7-3946. ApJ 708:965-980 (2010)
Acknowledgements
I would like to acknowledge the support of everyone involved in preparing this review, in particular the Fermi-LAT, H.E.S.S., and CTA collaborations.
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2016 Springer International Publishing AG
About this entry
Cite this entry
Funk, S. (2016). High-Energy Gamma Rays from Supernova Remnants. In: Alsabti, A., Murdin, P. (eds) Handbook of Supernovae. Springer, Cham. https://doi.org/10.1007/978-3-319-20794-0_12-1
Download citation
DOI: https://doi.org/10.1007/978-3-319-20794-0_12-1
Received:
Accepted:
Published:
Publisher Name: Springer, Cham
Online ISBN: 978-3-319-20794-0
eBook Packages: Springer Reference Physics and AstronomyReference Module Physical and Materials ScienceReference Module Chemistry, Materials and Physics