Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-17T14:04:09.907Z Has data issue: false hasContentIssue false
  • English
  • Français

Modeling the Radio and X-ray Emission of SN 1993J and SN 2002ap

Published online by Cambridge University Press:  19 September 2016

Claes Fransson  and
Claes-Ingvar Björnsson
Claes Fransson
Affiliation:
Department of Astronomy, Stockholm University, AlbaNova, 106 91 Stockholm, [email protected], [email protected]
Claes-Ingvar Björnsson
Affiliation:
Department of Astronomy, Stockholm University, AlbaNova, 106 91 Stockholm, [email protected], [email protected]

Summary

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Modeling of radio and X-ray observations of supernovae interacting with their circumstellar media are discussed, with special application to SN 1993J and SN 2002ap. We emphasize the importance of including all relevant physical mechanisms, especially for the modeling of the radio light curves. The different conclusions for the absorption mechanism (free-free or synchrotron self-absorption), as well as departures from an ρ ∝ r−2 CSM, as inferred by some authors, are discussed in detail. We conclude that the evidence for a variation in the mass loss rate with time is very weak. The results regarding the efficiencies of magnetic field generation and relativistic particle acceleration are summarized.

Type
Part I Supernovae: Individual
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 59 - 69
Copyright
Copyright © Springer-Verlag 2005

References

1. Bartel, N. et al.: Science 287, 112 (2000)Google Scholar
2. Berger, E., Kulkami, S.R., Chevalier, R.A.: Astrophys. J.Lett. 577, L5 (2002)Google Scholar
3. Björnsson, C.-I., Fransson, C.: astro-ph 0401196 (2004)Google Scholar
4. Chandra, P., Ray, A., Bhatnagar, S.: astro-ph 0402391 (2004)Google Scholar
5. Chevalier, R.A.: Astrophys. J. 258, 790 (1982)Google Scholar
6. Chevalier, R.A.: Astrophys. J. 499, 810 (1998)Google Scholar
7. Chevalier, R.A., Fransson, C.: Astrophys. J. 420, 268 (1994)CrossRefGoogle Scholar
8. Chevalier, R.A., Fransson, C.: In: Supernovae and Gamma-Ray Bursters, LNP 598, ed. Weiler, K. (Springer: Berlin 2003) p. 171 Google Scholar
9. Ensman, L., Burrows, A.: Astrophys. J. 393, 742 (1992)Google Scholar
10. Fransson, C.: Astron. Astrophys. 133, 264 (1984)Google Scholar
11. Fransson, C., Björnsson, C.-I.: Astrophys. J. 509, 861 (1998)Google Scholar
12. Fransson, C. Lundqvist, P., Chevalier, R.A.: Astrophys. J. 461, 993 (1996)Google Scholar
13. Frederiksen, J.T., Hededal, C.B., Haugboelle, T., Nordlund, A.: astro-ph 0308104 (2003)Google Scholar
14. Heger, A., Jeannin, L., Langer, N., Bararle, I.: Astron. Astrophys. 327, 224 (1997)Google Scholar
15. Immler, S., Aschenbach, B., Wang, Q.D.: Astrophys. J. Lett. 561, L107 (2001)Google Scholar
16. Iwamoto, K., Young, T.R., Nakasato, N., Shigeyama, T., Nomoto, K., Hachisu, I., Saio, H.: Astrophys. J. 477, 865 (1997)Google Scholar
17. Kulkami, S.R. et al.: Nature 395, 663 (1998)Google Scholar
18. Leising, M.D. et al.: Astrophys. J. Lett. 431, L95 (1994)Google Scholar
19. Li, Z., Chevalier, R.A.: Astrophys. J. 526, 716 (1999)Google Scholar
20. Lundqvist, P., Fransson, C.: Astron. Astrophys. 192, 221 (1988)Google Scholar
21. Lundqvist, P., Fransson, C.: Astrophys. J. 380, 575 (1991)Google Scholar
22. Lundqvist, P., Fransson, C.: Astrophys. J. 464, 924 (1996)Google Scholar
23. Marcaide, J.M. et al.: Astrophys. J. Lett. 486, L31 (1997)Google Scholar
24. Matzner, C.D., Mckee, C.F.: Astrophys. J. 510, 379 (1999)Google Scholar
25. Mazzali, P.A. et al.: Astrophys. J. Lett. 572, L61 (2002)Google Scholar
26. Medvedev, M.V., Loeb, A.: Astrophys. J. 526, 697 (1999)Google Scholar
27. Meynet, G., Maeder, A.: Astron. Astrophys. 404, 975 (2003)Google Scholar
28. Nakamura, T., Mazzali, P.A., Nomoto, K., Iwamoto, K.: Astrophys. J. 550, 991 (2001)Google Scholar
29. Nishikawa, K.-I., Hardec, P., Richardson, G., Preece, R., Sol, H., Fishman, G.J.: astro-ph 0305091 (2003)Google Scholar
30. Nugis, T., Lamers, H.J.G.L.M.: Astron. Astrophys. 360, 227 (2000)Google Scholar
31. Pérez-Torres, M.A., Alberdi, A., Marcaide, J.M.: Astron. Astrophys. 374, 997 (2001)Google Scholar
32. Pérez-Torres, M.A., Alberdi, A., Marcaide, J.M.: Astron. Astrophys. 394, 71 (2002)Google Scholar
33. Soria, P., Pian, E., Mazzali, P.: Astron. Astrophys. 413, 107 (2004)Google Scholar
34. Sutaria, F.K., Chandra, P., Bhatnagar, S., Ray, A.: Astron. Astrophys. 397, 1011 (2003)Google Scholar
35. Swartz, D.A., Ghosh, K.K., McCollough, M.L., Pannuti, T.G., Tennant, A.F., Wu, K.: Astrophys. J. Suppl. 144, 213 (2003)Google Scholar
36. Suzuki, T., Nomoto, K.: Astrophys. J. 455, 658 (1995)Google Scholar
37. Uno, S. et al.: Astrophys. J. 565, 419 (2002)Google Scholar
38. Van Dyk, S.D., Weiler, K.W., Sramek, R.A., Rupen, M.P., Panagia, N.: Astrophys. J. Lett. 432, L115 (1994)Google Scholar
39. Zimmermann, H.U. et al.: Nature 367, 621 (1994)Google Scholar
40. Zimmermann, H.U., Aschenbach, B.: Astron. Astrophys. 406, 969 (2003)Google Scholar