Acero, F. et al. (June 2010). “First detection of VHE γ-rays from SN 1006 by HESS”. In: A&A 516, A62, A62. DOI: 10 .1051/0004-6361 / 200913916. arXiv: 1004.2124 [astro-ph.HE].
Acero, F. et al. (May 2016). “The First Fermi LAT Supernova Remnant Cat- alog”. In: ApJS 224, 8, p. 8. DOI: 10.3847/0067-0049/224/1/8. arXiv: 1511.06778 [astro-ph.HE].
Ackermann, M. et al. (Feb. 2013). “Detection of the Characteristic Pion-Decay Signature in Supernova Remnants”. In: Science 339, pp. 807–811. DOI: 10. 1126/science.1231160. arXiv: 1302.3307 [astro-ph.HE].
Adams, Scott M. et al. (Dec. 2013). “Observing the Next Galactic Supernova”. In: ApJ 778.2, 164, p. 164. DOI: 10.1088/0004-637X/778/2/164. arXiv:1306.0559 [astro-ph.HE].
Aguilar, M. et al. (Nov. 2015a). “Precision Measurement of the Helium Flux in Primary Cosmic Rays of Rigidities 1.9 GV to 3 TV with the Alpha Mag- netic Spectrometer on the International Space Station”. In: PhRvL 115.21, 211101, p. 211101. DOI: 10.1103/PhysRevLett.115.211101.
Aguilar, M. et al. (May 2015b). “Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Mag- netic Spectrometer on the International Space Station”. In: PhRvL 114.17, 171103, p. 171103. DOI: 10.1103/PhysRevLett.114.171103.
Aguilar, M. et al. (Dec. 2017). “Observation of the Identical Rigidity Depen- dence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Mag- netic Spectrometer on the International Space Station”. In: PhRvL 119.25, 251101, p. 251101. DOI: 10.1103/PhysRevLett.119.251101.
Aharonian, F. et al. (Mar. 2007). “Primary particle acceleration above 100 TeV in the shell-type supernova remnant <ASTROBJ>RX J1713.7-3946</ASTROBJ> with deep HESS observations”. In: A&A 464, pp. 235–243. DOI: 10.1051/0004-6361:20066381. eprint: astro-ph/0611813.
Aharonian, F. et al. (Sept. 2008). “HESS upper limits for Kepler’s supernova remnant”. In: A&A 488, pp. 219–223. DOI: 10.1051/0004-6361:200809401. arXiv: 0806.3347.
Aharonian, F. et al. (July 2011). “Primary particle acceleration above 100 TeV in the shell-type supernova remnant RX J1713.7 - 3946 with deep H.E.S.S. observations (Corrigendum)”. In: A&A 531, C1, p. C1. DOI: 10 . 1051 / 0004-6361/20066381e.
Aharonian, F. A., S. R. Kelner, and A. Y. Prosekin (Aug. 2010). “Angular, spectral, and time distributions of highest energy protons and associated secondary gamma rays and neutrinos propagating through extragalactic magnetic and radiation fields”. In: PhRvD 82.4, 043002, p. 043002. DOI: 10.1103/PhysRevD.82.043002. arXiv: 1006.1045 [astro-ph.HE].
Ahnen, M. L. et al. (Dec. 2017). “A cut-off in the TeV gamma-ray spectrum of the SNR Cassiopeia A”. In: MNRAS 472, pp. 2956–2962. DOI: 10.1093/ mnras/stx2079. arXiv: 1707.01583 [astro-ph.HE].
Albert, J. et al. (Aug. 2007). “Discovery of Very High Energy Gamma Radia- tion from IC 443 with the MAGIC Telescope”. In: ApJL 664, pp. L87–L90. DOI: 10.1086/520957. arXiv: 0705.3119.
Allen, G. E., R. Petre, and E. V. Gotthelf (Sept. 2001). “X-Ray Synchrotron Emission from 10-100 TeV Cosmic-Ray Electrons in the Supernova Rem- nant SN 1006”. In: ApJ 558, pp. 739–752. DOI: 10.1086/322470. eprint: astro-ph/0107540.
Allen, G. E. et al. (Jan. 2015). “On the Expansion Rate, Age, and Distance of the Supernova Remnant G266.2-1.2 (Vela Jr.)” In: ApJ 798, 82, p. 82. DOI: 10.1088/0004-637X/798/2/82. arXiv: 1410.7435 [astro-ph.HE].
Amato, E. and P. Blasi (Feb. 2009). “A kinetic approach to cosmic-ray-induced streaming instability at supernova shocks”. In: MNRAS 392.4, pp. 1591– 1600. DOI: 10 . 1111 / j . 1365 - 2966 . 2008 . 14200 . x. arXiv: 0806 . 1223 [astro-ph].
Ambrocio-Cruz, P. et al. (Nov. 2017). “Kinematic study at the H α line in the north-eastern region of the Galactic supernova remnant IC 443”. In: MN- RAS 472, pp. 51–54. DOI: 10.1093/mnras/stx1936.
Archambault, S. et al. (Feb. 2017). “Gamma-Ray Observations of Tycho’s Su- pernova Remnant with VERITAS and Fermi”. In: ApJ 836, 23, p. 23. DOI: 10.3847/1538-4357/836/1/23. arXiv: 1701.06740 [astro-ph.HE].
Artyukh, V. S., V. V. Vitkevich, and R. D. Dagkesamanskii (1967). “Radio- Source Spectra at Meter Wavelengths.” In: AZh 44, p. 984.
Baade, W. and F. Zwicky (May 1934). “Cosmic Rays from Super-novae”. In: Proceedings of the National Academy of Science 20, pp. 259–263. DOI: 10 . 1073/pnas.20.5.259.
Ballet, J. et al. (May 2020). “Fermi Large Area Telescope Fourth Source Cata- log Data Release 2”. In: arXiv e-prints, arXiv:2005.11208, arXiv:2005.11208. arXiv: 2005.11208 [astro-ph.HE].
Bamba, A. et al. (Jan. 2008). “Suzaku Wide-Band Observations of SN1006”. In: PASJ 60, S153–S162. DOI: 10.1093/pasj/60.sp1.S153. arXiv: 0708.0073.
Baring, M. G. et al. (Mar. 1999). “Radio to Gamma-Ray Emission from Shell- Type Supernova Remnants: Predictions from Nonlinear Shock Acceler- ation Models”. In: ApJ 513, pp. 311–338. DOI: 10 .1086 / 306829. eprint: astro-ph/9810158.
Bell, A. R. (Jan. 1978a). “The acceleration of cosmic rays in shock fronts. I”. In: MNRAS 182, pp. 147–156. DOI: 10.1093/mnras/182.2.147.
— (Feb. 1978b). “The acceleration of cosmic rays in shock fronts. II”. In: MN- RAS 182, pp. 443–455. DOI: 10.1093/mnras/182.3.443.
— (Sept. 2004). “Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays”. In: MNRAS 353, pp. 550–558. DOI: 10.1111/ j.1365-2966.2004.08097.x.
Biermann, Peter L. et al. (Dec. 2010). “The Origin of Cosmic Rays: Explosions of Massive Stars with Magnetic Winds and Their Supernova Mechanism”. In: ApJ 725.1, pp. 184–187. DOI: 10.1088/0004-637X/725/1/184. arXiv: 1009.5592 [astro-ph.HE].
Blandford, R. D. and J. P. Ostriker (Apr. 1978). “Particle acceleration by astro- physical shocks”. In: ApJL 221, pp. L29–L32. DOI: 10.1086/182658.
Blasi, P. (Apr. 2004). “Nonlinear shock acceleration in the presence of seed particles”. In: Astroparticle Physics 21, pp. 45–57. DOI: 10.1016/j.astropartphys. 2003.10.008. eprint: astro-ph/0310507.
Blasi, P., S. Gabici, and G. Vannoni (Aug. 2005). “On the role of injection in kinetic approaches to non-linear particle acceleration at non-relativistic shock waves”. In: MNRAS 361, pp. 907–918. DOI: 10.1111/j.1365-2966. 2005.09227.x. eprint: astro-ph/0505351.
Blondin, J. M. and D. C. Ellison (Oct. 2001). “Rayleigh-Taylor Instabilities in Young Supernova Remnants Undergoing Efficient Particle Acceleration”. In: ApJ 560, pp. 244–253. DOI: 10.1086/322499. eprint: astro-ph/0104024.
Blumenthal, George R. and Robert J. Gould (Jan. 1970). “Bremsstrahlung, Synchrotron Radiation, and Compton Scattering of High-Energy Electrons Traversing Dilute Gases”. In: Reviews of Modern Physics 42.2, pp. 237–271. DOI: 10.1103/RevModPhys.42.237.
Borkowski, Kazimierz et al. (Aug. 1996). “A Circumstellar Shell Model for the Cassiopeia A Supernova Remnant”. In: ApJ 466, p. 866. DOI: 10.1086/ 177560.
Caprioli, D., E. Amato, and P. Blasi (June 2010). “Non-linear diffusive shock acceleration with free-escape boundary”. In: Astroparticle Physics 33, pp. 307–311. DOI: 10.1016/j.astropartphys.2010.03.001. arXiv: 0912.2714 [astro-ph.HE].
Caprioli, D., P. Blasi, and E. Amato (July 2009). “On the escape of particles from cosmic ray modified shocks”. In: MNRAS 396, pp. 2065–2073. DOI: 10.1111/j.1365-2966.2008.14298.x. arXiv: 0807.4259.
Caprioli, D. et al. (May 2009). “Dynamical feedback of self-generated mag- netic fields in cosmic ray modified shocks”. In: MNRAS 395, pp. 895–906. arXiv: 0807.4261.
Caprioli, D. et al. (Sept. 2010). “Comparison of different methods for non- linear diffusive shock acceleration”. In: MNRAS 407, pp. 1773–1783. DOI: 10.1111/j.1365-2966.2010.17013.x. arXiv: 1005.2127 [astro-ph.HE].
Carlton, A. K. et al. (Aug. 2011). “Expansion of the Youngest Galactic Super- nova Remnant G1.9+0.3”. In: ApJL 737, L22, p. L22. DOI: 10.1088/2041- 8205/737/1/L22. arXiv: 1106.4498.
Case, Gary L. and Dipen Bhattacharya (Sept. 1998). “A New Σ-D Relation and Its Application to the Galactic Supernova Remnant Distribution”. In: ApJ 504.2, pp. 761–772. DOI: 10.1086/306089. arXiv: astro-ph/9807162 [astro-ph].
Castelletti, G. et al. (Aug. 2007). “The low-frequency radio emission and spec- trum of the extended SNR <ASTROBJ>W44</ASTROBJ>: new VLA ob- servations at 74 and 324 MHz”. In: A&A 471, pp. 537–549. DOI: 10.1051/0004-6361:20077062. eprint: astro-ph/0702746.
Castelletti, G. et al. (Oct. 2011). “High-resolution radio study of SNR IC 443 at low radio frequencies”. In: A&A 534, A21, A21. DOI: 10.1051/0004- 6361/201016081. arXiv: 1104.0205.
Cherenkov Telescope Array Consortium et al. (2019). Science with the Cherenkov Telescope Array. DOI: 10.1142/10986.
Chevalier, R. A. (Aug. 1982a). “Are young supernova remnants interacting with circumstellar gas”. In: ApJL 259, pp. L85–L89. DOI: 10.1086/183853.
— (July 1982b). “Self-similar solutions for the interaction of stellar ejecta with an external medium”. In: ApJ 258, pp. 790–797. DOI: 10.1086/160126.
— (Sept. 1983). “Blast waves with cosmic-ray pressure”. In: ApJ 272, pp. 765– 772. DOI: 10.1086/161338.
Chevalier, Roger A. and Claes Fransson (Nov. 2006). “Circumstellar Emission from Type Ib and Ic Supernovae”. In: ApJ 651.1, pp. 381–391. DOI: 10 . 1086/507606. arXiv: astro-ph/0607196 [astro-ph].
Clark, D. H. and J. L. Caswell (Feb. 1976). “A study of galactic supernova remnants, based on Molonglo-Parkes observational data.” In: MNRAS 174, pp. 267–305. DOI: 10.1093/mnras/174.2.267.
Condon, B. et al. (Dec. 2017). “Detection of Two TeV Shell-type Remnants at GeV Energies with FERMI LAT: HESS J1731-347 and SN 1006”. In: ApJ 851, 100, p. 100. DOI: 10.3847/1538- 4357/aa9be8. arXiv: 1711.05499 [astro-ph.HE].
DeLaney, T. and L. Rudnick (June 2003). “The First Measurement of Cas- siopeia A’s Forward Shock Expansion Rate”. In: ApJ 589, pp. 818–826. DOI: 10.1086/374813. eprint: astro-ph/0303399.
Devin, J. et al. (Nov. 2020). “High-energy gamma-ray study of the dynam- ically young SNR G150.3+4.5”. In: A&A 643, A28, A28. DOI: 10 .1051 / 0004-6361/202038503. arXiv: 2009.08397 [astro-ph.HE].
Drury, L. (Sept. 1983). “On particle acceleration in supernova remnants”. In: SSRv 36, pp. 57–60. DOI: 10.1007/BF00171901.
Duncan, A. R. and D. A. Green (Dec. 2000). “The supernova remnant RX J0852.0-4622: radio characteristics and implications for SNR statistics”. In: A&A 364, pp. 732–740. eprint: astro-ph/0009289.
Dwarkadas, V. V. and R. A. Chevalier (Apr. 1998). “Interaction of Type IA Supernovae with Their Surroundings”. In: ApJ 497, pp. 807–823. DOI: 10. 1086/305478.
Elias, J. H. et al. (Sept. 1985). “Type I supernovae in the infrared and their use as distance indicators.” In: ApJ 296, pp. 379–389. DOI: 10.1086/163456.
Ellison, D. C. et al. (Jan. 2012). “Core-collapse Model of Broadband Emission from SNR RX J1713.7-3946 with Thermal X-Rays and Gamma Rays from Escaping Cosmic Rays”. In: ApJ 744, 39, p. 39. DOI: 10.1088/0004-637X/ 744/1/39. arXiv: 1109.0874 [astro-ph.HE].
Ertl, T. et al. (Feb. 2020). “The Explosion of Helium Stars Evolved with Mass Loss”. In: ApJ 890.1, 51, p. 51. DOI: 10.3847/1538-4357/ab6458. arXiv: 1910.01641 [astro-ph.HE].
Fang, J. and L. Zhang (Mar. 2008). “Non-thermal emission from old super- nova remnants”. In: MNRAS 384, pp. 1119–1128. DOI: 10.1111/j.1365- 2966.2007.12766.x. arXiv: 0711.4173.
Fermi, E. (Apr. 1949). “On the Origin of the Cosmic Radiation”. In: Physical Review 75, pp. 1169–1174. DOI: 10.1103/PhysRev.75.1169.
Ferrand, G. and S. Safi-Harb (May 2012). “A census of high-energy observa- tions of Galactic supernova remnants”. In: Advances in Space Research 49, pp. 1313–1319. DOI: 10 .1016 / j.asr.2012 .02 .004. arXiv: 1202 .0245 [astro-ph.HE].
Filippenko, Alexei V. (Jan. 1997). “Optical Spectra of Supernovae”. In: ARA&A 35, pp. 309–355. DOI: 10.1146/annurev.astro.35.1.309.
Fukui, Y. et al. (Feb. 2012). “A Detailed Study of the Molecular and Atomic Gas toward the γ-Ray Supernova Remnant RX J1713.7-3946: Spatial TeV γ-Ray and Interstellar Medium Gas Correspondence”. In: ApJ 746, 82, p. 82. DOI: 10.1088/0004-637X/746/1/82. arXiv: 1107.0508.
Gaensler, B. M. and B. J. Wallace (Sept. 2003). “A Multifrequency Radio Study of Supernova Remnant G292.0+1.8 and Its Pulsar Wind Nebula”. In: ApJ 594, pp. 326–339. DOI: 10.1086/376861. eprint: astro-ph/0305168.
Gaggero, D. et al. (Apr. 2018). “Time evolution of gamma rays from super- nova remnants”. In: MNRAS 475, pp. 5237–5245. DOI: 10.1093/mnras/ sty140. arXiv: 1710.05038 [astro-ph.HE].
Ginzburg, V. L. and S. I. Syrovatskii (1964). The Origin of Cosmic Rays. Giordano, F. et al. (Jan. 2012). “Fermi Large Area Telescope Detection of the Young Supernova Remnant Tycho”. In: ApJL 744, L2, p. L2. DOI: 10.1088/ 2041-8205/744/1/L2. arXiv: 1108.0265 [astro-ph.HE].
Giuliani, A. et al. (Dec. 2011). “Neutral Pion Emission from Accelerated Pro- tons in the Supernova Remnant W44”. In: ApJL 742, L30, p. L30. DOI: 10.1088/2041-8205/742/2/L30. arXiv: 1111.4868 [astro-ph.HE].
Gök, F. and A. Sezer (Jan. 2012). “Ejecta detection in the middle-aged Galactic supernova remnant G296.1-0.5 observed with Suzaku”. In: MNRAS 419, pp. 1603–1609. DOI: 10.1111/j.1365-2966.2011.19822.x. arXiv: 1109. 3971 [astro-ph.HE].
Gonzalez, M. and S. Safi-Harb (Feb. 2003). “New Constraints on the Energet- ics, Progenitor Mass, and Age of the Supernova Remnant G292.0+1.8 Con- taining PSR J1124-5916”. In: ApJL 583, pp. L91–L94. DOI: 10.1086/368122. eprint: astro-ph/0301193.
Green, D. A. (June 2017). “VizieR Online Data Catalog: A Catalogue of Galac- tic Supernova Remnants (Green 2017)”. In: VizieR Online Data Catalog, VII/278, pp. VII/278.
Gvaramadze, V. V. et al. (Apr. 2017). “IRAS 18153-1651: an H II region with a possible wind bubble blown by a young main-sequence B star”. In: MN- RAS 466.2, pp. 1857–1867. DOI: 10.1093/mnras/stw3257. arXiv: 1612. 03916 [astro-ph.SR].
H. E. S. S. Collaboration et al. (Feb. 2015). “H.E.S.S. reveals a lack of TeV emission from the supernova remnant Puppis A”. In: A&A 575, A81, A81. DOI: 10.1051/0004-6361/201424805. arXiv: 1412.6997 [astro-ph.HE].
H. E. S. S. Collaboration et al. (Apr. 2018). “H.E.S.S. observations of RX J1713.7- 3946 with improved angular and spectral resolution: Evidence for gamma- ray emission extending beyond the X-ray emitting shell”. In: A&A 612, A6, A6. DOI: 10.1051/0004-6361/201629790. arXiv: 1609.08671 [astro-ph.HE].
H. E. S. S. Collaboration et al. (Apr. 2018). “Population study of Galactic su- pernova remnants at very high γ-ray energies with H.E.S.S.” In: A&A 612, A3, A3. DOI: 10 .1051 /0004 - 6361 /201732125. arXiv: 1802 .05172 [astro-ph.HE].
Haug, E. (Sept. 1975). “Bremsstrahlung and pair production in the field of free electrons.” In: Zeitschrift Naturforschung Teil A 30, pp. 1099–1113. DOI: 10.1515/zna-1975-0901.
Helder, E. A. et al. (Oct. 2013). “Proper motions of Hα filaments in the su- pernova remnant RCW 86”. In: MNRAS 435, pp. 910–916. DOI: 10.1093/ mnras/stt993. arXiv: 1306.3994 [astro-ph.HE].
H.E.S.S. Collaboration et al. (June 2014). “TeV γ-ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with H.E.S.S.” In: MNRAS 441, pp. 790–799. DOI: 10.1093/mnras/stu459. arXiv: 1404.1613 [astro-ph.HE].
H.E.S.S. Collaboration et al. (Apr. 2018a). “Deeper H.E.S.S. observations of Vela Junior (RX J0852.0-4622): Morphology studies and resolved spec- troscopy”. In: A&A 612, A7, A7. DOI: 10.1051/0004- 6361/201630002. arXiv: 1611.01863 [astro-ph.HE].
H.E.S.S. Collaboration et al. (Apr. 2018b). “Detailed spectral and morpho- logical analysis of the shell type supernova remnant RCW 86”. In: A&A 612, A4, A4. DOI: 10 .1051 /0004 - 6361 /201526545. arXiv: 1601 .04461 [astro-ph.HE].
Hewitt, J. W. et al. (Nov. 2012). “Fermi-LAT and WMAP Observations of the Puppis A Supernova Remnant”. In: ApJ 759, 89, p. 89. DOI: 10.1088/0004- 637X/759/2/89.
Hui, C. Y. and W. Becker (Feb. 2009). “Exploring the X-ray emission proper- ties of the supernova remnant G67.7+1.8 and its central X-ray sources”. In: A&A 494, pp. 1005–1012. DOI: 10.1051/0004-6361:200810789. arXiv: 0812.2186.
Iłkiewicz, Krystian et al. (June 2019). “Wind Roche lobe overflow as a way to make Type Ia supernovae from the widest symbiotic systems”. In: MN- RAS 485.4, pp. 5468–5473. DOI: 10 . 1093 / mnras / stz760. arXiv: 1812 . 02602 [astro-ph.SR].
Jones, Frank C. (Mar. 1968). “Calculated Spectrum of Inverse-Compton-Scattered Photons”. In: Physical Review 167.5, pp. 1159–1169. DOI: 10.1103/PhysRev. 167.1159.
Kafexhiu, Ervin et al. (Dec. 2014). “Parametrization of gamma-ray produc- tion cross sections for p p interactions in a broad proton energy range from the kinematic threshold to PeV energies”. In: PhRvD 90.12, 123014, p. 123014. DOI: 10.1103/PhysRevD.90.123014. arXiv: 1406.7369 [astro-ph.HE].
Kamae, T. et al. (Aug. 2006). “Parameterization of γ, e+/−, and Neutrino Spectra Produced by p-p Interaction in Astronomical Environments”. In: ApJ 647, pp. 692–708. DOI: 10.1086/505189. eprint: astro-ph/0605581.
Kasen, Daniel and S. E. Woosley (Oct. 2009). “Type II Supernovae: Model Light Curves and Standard Candle Relationships”. In: ApJ 703.2, pp. 2205– 2216. DOI: 10.1088/0004-637X/703/2/2205. arXiv: 0910.1590 [astro-ph.CO].
Katsuda, S. et al. (Feb. 2010). “X-ray Measured Dynamics of Tycho’s Super- nova Remnant”. In: ApJ 709, pp. 1387–1395. DOI: 10.1088/0004-637X/709/2/1387. arXiv: 1001.2484 [astro-ph.HE].
Katsuda, Satoru et al. (Nov. 2015). “Evidence for Thermal X-Ray Line Emis- sion from the Synchrotron-dominated Supernova Remnant RX J1713.7- 3946”. In: ApJ 814.1, 29, p. 29. DOI: 10.1088/0004-637X/814/1/29. arXiv: 1510.04025 [astro-ph.HE].
Keohane, J. W. et al. (Jan. 2007). “A Near-Infrared and X-Ray Study of W49 B: A Wind Cavity Explosion”. In: ApJ 654, pp. 938–944. DOI: 10.1086/ 509311. eprint: astro-ph/0609533.
Koch, H. W. and J. W. Motz (Oct. 1959). “Bremsstrahlung Cross-Section For- mulas and Related Data”. In: Reviews of Modern Physics 31.4, pp. 920–955. DOI: 10.1103/RevModPhys.31.920.
Kothes, R. et al. (Oct. 2006). “A catalogue of Galactic supernova remnants from the Canadian Galactic plane survey. I. Flux densities, spectra, and polarization characteristics”. In: A&A 457, pp. 1081–1093. DOI: 10.1051/ 0004-6361:20065062.
Koyama, K. et al. (Nov. 1995). “Evidence for shock acceleration of high-energy electrons in the supernova remnant SN1006”. In: Nature 378.6554, pp. 255–258. DOI: 10.1038/378255a0.
Krause, Oliver et al. (May 2008). “The Cassiopeia A Supernova Was of Type IIb”. In: Science 320.5880, p. 1195. DOI: 10.1126/science.1155788. arXiv: 0805.4557 [astro-ph].
Lazendic, J. S. et al. (Feb. 2004). “A High-Resolution Study of Nonthermal Radio and X-Ray Emission from Supernova Remnant G347.3-0.5”. In: ApJ 602, pp. 271–285. DOI: 10.1086/380956. eprint: astro-ph/0310696.
Lee, S.-H., D. C. Ellison, and S. Nagataki (May 2012a). “A Generalized Model of Nonlinear Diffusive Shock Acceleration Coupled to an Evolving Super- nova Remnant”. In: ApJ 750, 156, p. 156. arXiv: 1203.3614 [astro-ph.HE].
Lee, S.-H. et al. (June 2015). “Modeling Bright γ-Ray and Radio Emission at Fast Cloud Shocks”. In: ApJ 806, 71, p. 71. DOI: 10.1088/0004-637X/806/1/71. arXiv: 1504.05313 [astro-ph.HE].
Lee, Shiu-Hang, Donald C. Ellison, and Shigehiro Nagataki (May 2012b). “A Generalized Model of Nonlinear Diffusive Shock Acceleration Coupled to an Evolving Supernova Remnant”. In: ApJ 750.2, 156, p. 156. DOI: 10. 1088/0004-637X/750/2/156. arXiv: 1203.3614 [astro-ph.HE].
Li, Weidong et al. (June 2007). “On the Progenitors of Two Type II-P Super- novae in the Virgo Cluster”. In: ApJ 661.2, pp. 1013–1024. DOI: 10.1086/ 516747. arXiv: astro-ph/0701049 [astro-ph].
Lovchinsky, I. et al. (Apr. 2011). “A Chandra Observation of Supernova Rem- nant G350.1-0.3 and Its Central Compact Object”. In: ApJ 731, 70, p. 70. DOI: 10.1088/0004-637X/731/1/70. arXiv: 1102.5333 [astro-ph.HE].
Mackey, Jonathan et al. (Jan. 2015). “Wind bubbles within H ii regions around slowly moving stars”. In: A&A 573, A10, A10. DOI: 10.1051/0004-6361/ 201424716. arXiv: 1410.0019 [astro-ph.GA].
Maeda, K. et al. (July 2015). “Type IIb Supernova 2013df Entering into an Interaction Phase: A Link between the Progenitor and the Mass Loss”. In: ApJ 807.1, 35, p. 35. DOI: 10.1088/0004-637X/807/1/35. arXiv: 1504. 06668 [astro-ph.SR].
Maeda, Y. et al. (Dec. 2009). “Suzaku X-Ray Imaging and Spectroscopy of Cassiopeia A”. In: PASJ 61, pp. 1217–1228. DOI: 10.1093/pasj/61.6.1217. arXiv: 0912.5020 [astro-ph.HE].
Matsumoto, Yosuke et al. (Sept. 2017). “Electron Surfing and Drift Accelera- tions in a Weibel-Dominated High-Mach-Number Shock”. In: Phys. Rev. Lett. 119 (10), p. 105101. DOI: 10.1103/PhysRevLett.119.105101. URL: https://link.aps.org/doi/10.1103/PhysRevLett.119.105101.
Matzner, Christopher D. and Christopher F. McKee (Jan. 1999). “The Expul- sion of Stellar Envelopes in Core-Collapse Supernovae”. In: ApJ 510.1, pp. 379–403. DOI: 10.1086/306571. arXiv: astro-ph/9807046 [astro-ph].
Mohamed, S., J. Mackey, and N. Langer (May 2012). “3D simulations of Betel- geuse’s bow shock”. In: A&A 541, A1, A1. DOI: 10 .1051/0004 - 6361 / 201118002. arXiv: 1109.1555 [astro-ph.SR].
Mohamed, S. and Ph. Podsiadlowski (Jan. 2012). “Mass Transfer in Mira-type Binaries”. In: Baltic Astronomy 21, pp. 88–96. DOI: 10.1515/astro-2017- 0362.
Nicholl, M. et al. (Oct. 2015). “On the diversity of superluminous supernovae: ejected mass as the dominant factor”. In: MNRAS 452, pp. 3869–3893. DOI: 10.1093/mnras/stv1522. arXiv: 1503.03310 [astro-ph.SR].
Nikolic´, S. et al. (Apr. 2013). “An Integral View of Fast Shocks Around Super- nova 1006”. In: Science 340, pp. 45–48. DOI: 10.1126/science.1228297. arXiv: 1302.4328 [astro-ph.HE].
Ohira, Yutaka and Kunihito Ioka (Mar. 2011). “Cosmic-ray Helium Harden- ing”. In: ApJL 729.1, L13, p. L13. DOI: 10.1088/2041-8205/729/1/L13.
Ouchi, Ryoma and Keiichi Maeda (May 2017). “Radii and Mass-loss Rates of Type IIb Supernova Progenitors”. In: ApJ 840.2, 90, p. 90. DOI: 10.3847/ 1538-4357/aa6ea9. arXiv: 1705.02430 [astro-ph.HE].
Planck Collaboration et al. (Feb. 2016). “Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants”. In: A&A 586, A134, A134. DOI: 10.1051/0004-6361/201425022. arXiv: 1409.5746.
Poveda, A. and L. Woltjer (Mar. 1968). “Supernovae and Supernova Rem- nants”. In: AJ 73, p. 65. DOI: 10.1086/110600.
Prinz, T. and W. Becker (Aug. 2012). “Exploring the supernova remnant G308.4-1.4”. In: A&A 544, A7, A7. DOI: 10.1051/0004-6361/201219086. arXiv: 1202.4677 [astro-ph.HE].
Ptuskin, Vladimir, Vladimir Zirakashvili, and Eun-Suk Seo (July 2010). “Spec- trum of Galactic Cosmic Rays Accelerated in Supernova Remnants”. In: ApJ 718.1, pp. 31–36. DOI: 10.1088/0004-637X/718/1/31. arXiv: 1006. 0034 [astro-ph.CO].
Rakowski, C. E., J. P. Hughes, and P. Slane (Feb. 2001). “Two New Ejecta- dominated Galactic Supernova Remnants: G337.2-0.7 and G309.2-0.6”. In: ApJ 548, pp. 258–268. DOI: 10.1086/318680. eprint: astro-ph/0010091.
Reynolds, M. T. et al. (Apr. 2013). “G306.3-0.9: A Newly Discovered Young Galactic Supernova Remnant”. In: ApJ 766, 112, p. 112. DOI: 10 .1088 / 0004-637X/766/2/112. arXiv: 1303.3546 [astro-ph.HE].
Reynoso, E. M., S. Cichowolski, and A. J. Walsh (Jan. 2017). “A high-resolution H I study towards the supernova remnant Puppis A and its environ- ments”. In: MNRAS 464, pp. 3029–3039. DOI: 10.1093/mnras/stw2219. arXiv: 1609.01779.
Roger, R. S. et al. (Apr. 1986). “G291.0-0.1, a centrally bright supernova rem- nant, in Carina”. In: MNRAS 219, pp. 815–822. DOI: 10.1093/mnras/219. 4.815.
Rybicki, George B. and Alan P. Lightman (1986). Radiative Processes in Astro- physics.
Sánchez-Ayaso, E. et al. (Apr. 2013). “XMM-Newton and Chandra observa- tions of G272.2-3.2. Evidence of stellar ejecta in the central region”. In: A&A 552, A52, A52. DOI: 10.1051/0004-6361/201219709. arXiv: 1301.1507 [astro-ph.HE].
Sasaki, M. et al. (Sept. 2018). “Infrared and X-ray study of the Galactic SNR G15.9+0.2”. In: MNRAS 479, pp. 3033–3041. DOI: 10.1093/mnras/sty1596. arXiv: 1806.11365 [astro-ph.HE].
Schinnerer, E. et al. (Nov. 2004). “The VLA-COSMOS Survey. I. Radio Iden- tifications from the Pilot Project”. In: AJ 128.5, pp. 1974–1989. DOI: 10 . 1086/424860. arXiv: astro-ph/0408149 [astro-ph].
Sedov, L. I. (1959). Similarity and Dimensional Methods in Mechanics.
Sezer, A., T. Ergin, and R. Yamazaki (Apr. 2017). “Suzaku analysis of the su- pernova remnant G306.3-0.9 and the gamma-ray view of its neighbour- hood”. In: MNRAS 466, pp. 3434–3441. DOI: 10 .1093 / mnras / stw3331.arXiv: 1701.00102 [astro-ph.HE].
Simpson, Chris et al. (Apr. 2012). “Radio imaging of the Subaru/XMM-Newton Deep Field- III. Evolution of the radio luminosity function beyond z= 1”. In: MNRAS 421.4, pp. 3060–3083. DOI: 10 .1111 / j.1365 - 2966 .2012 .20529.x. arXiv: 1201.3225 [astro-ph.CO].
Sinitsina, V. G. and V. Y. Sinitsina (June 2015). “Results of observations of shell supernova remnants at ultrahigh energies with the SHALON mir- ror Cherenkov telescopes”. In: Bulletin of the Lebedev Physics Institute 42, pp. 169–175. DOI: 10.3103/S1068335615060032. arXiv: 1602.01694 [astro-ph.HE].
Slane, P. et al. (Mar. 2014). “A CR-hydro-NEI Model of the Structure and Broadband Emission from Tycho’s Supernova Remnant”. In: ApJ 783, 33, p. 33. DOI: 10.1088/0004-637X/783/1/33. arXiv: 1401.2556 [astro-ph.HE].
Smartt, S. J. (Apr. 2015). “Observational Constraints on the Progenitors of Core-Collapse Supernovae: The Case for Missing High-Mass Stars”. In: PASA 32, e016, e016. DOI: 10.1017/pasa.2015.17. arXiv: 1504.02635 [astro-ph.SR].
Smith, Nathan (2017). “Interacting Supernovae: Types IIn and Ibn”. In: Hand- book of Supernovae. Ed. by Athem W. Alsabti and Paul Murdin, p. 403. DOI: 10.1007/978-3-319-21846-5\_38.
Smith, Nathan et al. (Apr. 2011). “Observed fractions of core-collapse super- nova types and initial masses of their single and binary progenitor stars”. In: MNRAS 412.3, pp. 1522–1538. DOI: 10 .1111 / j.1365 - 2966 .2011 .17229.x. arXiv: 1006.3899 [astro-ph.HE].
Spitzer, Lyman (1965). Physics of fully ionized gases.
Sturner, S. J. et al. (Dec. 1997). “Temporal Evolution of Nonthermal Spec- tra from Supernova Remnants”. In: ApJ 490, pp. 619–632. DOI: 10.1086/ 304894.
Sukhbold, Tuguldur and S. E. Woosley (Mar. 2014). “The Compactness of Presupernova Stellar Cores”. In: ApJ 783.1, 10, p. 10. DOI: 10.1088/0004- 637X/783/1/10. arXiv: 1311.6546 [astro-ph.SR].
Sukhbold, Tuguldur et al. (Apr. 2016). “Core-collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions”. In: ApJ 821.1, 38, p. 38. DOI: 10 .3847/0004-637X/821/1/38. arXiv: 1510 . 04643 [astro-ph.HE].
Sutherland, Ralph S. and M. A. Dopita (Sept. 1993). “Cooling Functions for Low-Density Astrophysical Plasmas”. In: ApJS 88, p. 253. DOI: 10.1086/ 191823.
Suzuki, Hiromasa et al. (Oct. 2020). “Study on the escape timescale of high- energy particles from supernova remnants through thermal X-ray prop- erties”. In: PASJ 72.5, 72, p. 72. DOI: 10.1093/pasj/psaa061. arXiv: 2006. 03382 [astro-ph.HE].
Tanaka, T. et al. (Oct. 2008). “Study of Nonthermal Emission from SNR RX J1713.7-3946 with Suzaku”. In: ApJ 685, pp. 988–1004. DOI: 10 . 1086 / 591020. arXiv: 0806.1490.
Tanaka, T. et al. (Oct. 2011). “Gamma-Ray Observations of the Supernova Remnant RX J0852.0-4622 with the Fermi Large Area Telescope”. In: ApJL 740, L51, p. L51. DOI: 10.1088/2041-8205/740/2/L51. arXiv: 1109.4658 [astro-ph.HE].
Tanaka, Takaaki et al. (Sept. 2020). “Shock-Cloud Interaction in the South- western Rim of RX J1713.7-3946 Evidenced by Chandra X-Ray Observa- tions”. In: ApJL 900.1, L5, p. L5. DOI: 10.3847/2041-8213/abaef0. arXiv: 2008.05581 [astro-ph.HE].
Tang, Z., S. P. Reynolds, and S. M. Ressler (Dec. 2016). “X-Ray and Gamma- Ray Emission from Middle-aged Supernova Remnants In cavities. I. Spher- ical Symmetry”. In: ApJS 227, 28, p. 28. DOI: 10.3847/1538-4365/227/2/28. arXiv: 1701.05615 [astro-ph.HE].
Tauris, Thomas M. and Gerrit J. Savonije (Oct. 1999). “Formation of millisec- ond pulsars. I. Evolution of low-mass X-ray binaries with P_orb> 2 days”. In: A&A 350, pp. 928–944. arXiv: astro-ph/9909147 [astro-ph].
Tavani, M. et al. (Feb. 2010). “Direct Evidence for Hadronic Cosmic-Ray Ac- celeration in the Supernova Remnant IC 443”. In: ApJL 710, pp. L151– L155. DOI: 10.1088/2041-8205/710/2/L151. arXiv: 1001.5150 [astro-ph.HE].
Townsend, R. H. D. (Apr. 2009). “An Exact Integration Scheme for Radiative Cooling in Hydrodynamical Simulations”. In: ApJS 181.2, pp. 391–397. DOI: 10.1088/0067-0049/181/2/391. arXiv: 0901.3146 [astro-ph.SR].
Troja, E. et al. (Dec. 2014). “Swift/BAT Detection of Hard X-Rays from Ty- cho’s Supernova Remnant: Evidence for Titanium-44”. In: ApJL 797, L6, p. L6. DOI: 10.1088/2041-8205/797/1/L6. arXiv: 1411.0991 [astro-ph.HE].
Truelove, J. K. and C. F. McKee (Feb. 1999). “Evolution of Nonradiative Su- pernova Remnants”. In: ApJS 120, pp. 299–326. DOI: 10.1086/313176.
Tsuji, N. and Y. Uchiyama (Dec. 2016). “Expansion measurements of super- nova remnant RX J1713.7-3946”. In: PASJ 68, 108, p. 108. DOI: 10.1093/pasj/psw102. arXiv: 1609.07886 [astro-ph.HE].
Uchida, H. et al. (Dec. 2012). “Recombining Plasma and Hard X-Ray Filament in the Mixed-Morphology Supernova Remnant W 44”. In: PASJ 64, 141, p. 141. DOI: 10.1093/pasj/64.6.141. arXiv: 1208.0113 [astro-ph.HE].
van den Heuvel, E. P. J. (Jan. 2009). “The Formation and Evolution of Rela- tivistic Binaries”. In: Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Ed. by Monica Colpi et al. Vol. 359. Astrophysics and Space Science Library, p. 125. DOI: 10.1007/978-1-4020-9264-0\_4.
Vartanyan, David et al. (July 2021). “Binary-stripped Stars as Core-collapse Supernovae Progenitors”. In: ApJL 916.1, L5, p. L5. DOI: 10.3847/2041- 8213/ac0b42. arXiv: 2104.03317 [astro-ph.SR].
Vink, J. (Dec. 2008). “The Kinematics of Kepler’s Supernova Remnant as Re- vealed by Chandra”. In: ApJ 689, pp. 231–241. DOI: 10 . 1086 / 592375. arXiv: 0803.4011.
Wang, Bo et al. (Sept. 2021). “Ultracompact X-ray binaries with He star com- panions”. In: MNRAS 506.3, pp. 4654–4666. DOI: 10.1093/mnras/stab2032. arXiv: 2106.01369 [astro-ph.HE].
Wang, C.-Y. and R. A. Chevalier (Mar. 2001). “Instabilities and Clumping in Type IA Supernova Remnants”. In: ApJ 549, pp. 1119–1134. DOI: 10.1086/ 319439. eprint: astro-ph/0005105.
Wang, W. and Z. Li (July 2016). “Hard X-Ray Emissions from Cassiopeia A Observed by INTEGRAL”. In: ApJ 825, 102, p. 102. DOI: 10.3847/0004-637X/825/2/102. arXiv: 1605.00360 [astro-ph.HE].
Warren, D. C. and J. M. Blondin (Mar. 2013). “Three-dimensional numeri- cal investigations of the morphology of Type Ia SNRs”. In: MNRAS 429, pp. 3099–3113. DOI: 10.1093/mnras/sts566. arXiv: 1210.7790.
Warren, J. S. et al. (Nov. 2005). “Cosmic-Ray Acceleration at the Forward Shock in Tycho’s Supernova Remnant: Evidence from Chandra X-Ray Ob- servations”. In: ApJ 634, pp. 376–389. DOI: 10.1086/496941. eprint: astro- ph/0507478.
Wheeler, J. Craig and Robert P. Harkness (Jan. 1986). “Physical models of su- pernovae and the distance scale.” In: Galaxy Distances and Deviations from Universal Expansion. Ed. by Barry F. Madore and R. Brent Tully. Vol. 180. NATO Advanced Study Institute (ASI) Series C, pp. 45–54.
Williams, B. J. et al. (June 2013). “Azimuthal Density Variations around the Rim of Tycho’s Supernova Remnant”. In: ApJ 770, 129, p. 129. DOI: 10. 1088/0004-637X/770/2/129. arXiv: 1305.0567 [astro-ph.HE].
Williams, B. J. et al. (Mar. 2018). “A Deep X-Ray View of the Synchrotron- dominated Supernova Remnant G330.2+1.0”. In: ApJ 855, 118, p. 118. DOI: 10.3847/1538-4357/aaadb6. arXiv: 1802.02804 [astro-ph.HE].
Woosley, S. E. (June 2019). “The Evolution of Massive Helium Stars, Including Mass Loss”. In: ApJ 878.1, 49, p. 49. DOI: 10.3847/1538- 4357/ab1b41. arXiv: 1901.00215 [astro-ph.SR].
Woosley, S. E. and A. Heger (Apr. 2007). “Nucleosynthesis and remnants in massive stars of solar metallicity”. In: PhR 442.1-6, pp. 269–283. DOI: 10. 1016/j.physrep.2007.02.009. arXiv: astro-ph/0702176 [astro-ph].
Woosley, S. E. and Alexander Heger (Sept. 2015). “The Remarkable Deaths of 9-11 Solar Mass Stars”. In: ApJ 810.1, 34, p. 34. DOI: 10.1088/0004-637X/810/1/34. arXiv: 1505.06712 [astro-ph.SR].
Woosley, S. E., Tuguldur Sukhbold, and H. T. Janka (June 2020). “The Birth Function for Black Holes and Neutron Stars in Close Binaries”. In: ApJ 896.1, 56, p. 56. DOI: 10 .3847 / 1538 - 4357 / ab8cc1. arXiv: 2001 .10492 [astro-ph.HE].
Woosley, S. E., Tuguldur Sukhbold, and D. N. Kasen (June 2021). “Model Light Curves for Type Ib and Ic Supernovae”. In: ApJ 913.2, 145, p. 145. DOI: 10.3847/1538-4357/abf3be. arXiv: 2009.06868 [astro-ph.HE].
Xin, Y.-L. et al. (July 2017). “Revisiting SNR Puppis A with Seven Years of Fermi Large Area Telescope Observations”. In: ApJ 843, 90, p. 90. DOI: 10.3847/1538-4357/aa74bb. arXiv: 1703.03911 [astro-ph.HE].
Yasuda, Haruo and Shiu-Hang Lee (May 2019). “Time Evolution of Broad- band Nonthermal Emission from Supernova Remnants in Different Cir- cumstellar Environments”. In: ApJ 876.1, 27, p. 27. DOI: 10.3847/1538- 4357/ab13ab. arXiv: 1903.10226 [astro-ph.HE].
Yasuda, Haruo, Shiu-Hang Lee, and Keiichi Maeda (Oct. 2021). “Dark Age of Type II Supernova Remnants”. In: ApJL 919.2, L16, p. L16. DOI: 10.3847/ 2041-8213/ac24ac. arXiv: 2109.04032 [astro-ph.HE].
Yoon, Sung-Chul (Oct. 2017). “Towards a better understanding of the evolu- tion of Wolf-Rayet stars and Type Ib/Ic supernova progenitors”. In: MN- RAS 470.4, pp. 3970–3980. DOI: 10.1093/mnras/stx1496. arXiv: 1706. 04716 [astro-ph.SR].
Yuan, Q., S. Liu, and X. Bi (Dec. 2012). “An Attempt at a Unified Model for the Gamma-Ray Emission of Supernova Remnants”. In: ApJ 761, 133, p. 133. DOI: 10.1088/0004-637X/761/2/133. arXiv: 1203.0085 [astro-ph.HE].
Yuan, Yajie et al. (Dec. 2013). “Fermi Large Area Telescope Detection of a Break in the Gamma-Ray Spectrum of the Supernova Remnant Cassiopeia A”. In: ApJ 779.2, 117, p. 117. DOI: 10.1088/0004-637X/779/2/117. arXiv: 1310.8287 [astro-ph.HE].
Zhu, H., W. W. Tian, and P. Zuo (Oct. 2014). “Supernova Remnant W49B and Its Environment”. In: ApJ 793, 95, p. 95. DOI: 10.1088/0004-637X/793/2/95. arXiv: 1407.8260 [astro-ph.SR].
Zirakashvili, V. N. and V. S. Ptuskin (Dec. 2012). “Numerical simulations of diffusive shock acceleration in SNRs”. In: Astroparticle Physics 39, pp. 12–21. DOI: 10 .1016 / j.astropartphys .2011 .09 .003. arXiv: 1109 .4482 [astro-ph.HE].