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A Decade of Radio and X-ray Observations of SN 1993J

Published online by Cambridge University Press:  19 September 2016

Schuyler D. Van Dyk ,
Kurt W. Weiler ,
Richard A. Sramek ,
Nino Panagia ,
Christopher Stockdale ,
Christina Lacey ,
Marcos Montes  and
Michael Rupen
Schuyler D. Van Dyk
Affiliation:
IPAC/Caltech, Pasadena, CA, USA; vandyk@ipac.caltech.edu
Kurt W. Weiler
Affiliation:
NRL, Washington, DC, USA; Kurt.Weiler@nrl.navy.mil, Marcos.Montes@nrl.navy.mil
Richard A. Sramek
Affiliation:
NRAO, Socorro, NM, USA; dsramek@aoc.nrao.edu, mrupen@aoc.nrao.edu
Nino Panagia
Affiliation:
STScI, Baltimore, MD, USA& Astrophys. Div., Space Sci. Dept., ESA; , panagia@stsci.edu
Christopher Stockdale
Affiliation:
Marquette Univ., Milwaukee, WI, USA; Christopher.Stockdale@marquette.edu
Christina Lacey
Affiliation:
U. of South Carolina, Columbia, SC, USA; lacey@sc.edu
Marcos Montes
Affiliation:
NRL, Washington, DC, USA; Kurt.Weiler@nrl.navy.mil, Marcos.Montes@nrl.navy.mil
Michael Rupen
Affiliation:
NRAO, Socorro, NM, USA; dsramek@aoc.nrao.edu, mrupen@aoc.nrao.edu

Summary

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We review ten years of radio continuum and X-ray monitoring of the Type IIb SN 1993J in M81. The supernova (SN) has been observed continuously, since only a few days after explosion, by our group with the Very Large Array at a number of radio frequencies, as well as by other groups. As a result, it is among the best-studied radio supernovae. The observed synchrotron radio emission is thought to arise from the interaction of the SN shock with the pre-SN wind-established circumstellar medium around the progenitor star. We describe the properties of the circumstellar interaction, based on the more fully-developed dataset, and compare this to our earlier characterization made in 1994. SN 1993J has also been a target of X-ray satellites, and we briefly discuss the nature of the X-ray emission and, together with the radio emission, describe the implications for the nature of the SN’s progenitor.

Type
Part I Supernovae: Individual
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 3 - 11
Copyright
Copyright © Springer-Verlag 2005

References

1. Bartel, N. et al.: Nature 368, 610 (1994)CrossRefGoogle Scholar
2. Bartel, N. et al.: Astrophys. J. 581, 404 (2002)CrossRefGoogle Scholar
3. Chevalier, R.A.: Astrophys. J. 259, 302 (1982)CrossRefGoogle Scholar
4. Chevalier, R.A.: Astrophys. J. Lett. 258, L63 (1984)CrossRefGoogle Scholar
5. Chevalier, R.A.: Astrophys. J. 499, 810 (1998)CrossRefGoogle Scholar
6. Chevalier, R.A., Fransson, C.: Astrophys. J. 420, 268 (1994)CrossRefGoogle Scholar
7. Fransson, C., Lundqvist, P., Chevalier, R.A.: Astrophys. J. 461, 993 (1996)CrossRefGoogle Scholar
8. Fransson, C., Björnsson, C.-I.: Astrophys. J. 509, 861 (1998)CrossRefGoogle Scholar
9. Immler, S., Aschenbach, B., Wang, Q.D.: Astrophys. J. Lett. 561, L107 (2001)CrossRefGoogle Scholar
10. Kohmura, Y. et al.: Pub. Astron. Soc. Japan 46, L157 (1994)Google Scholar
11. Leising, M.D. et al.: Astrophys. J. Lett. 431, L95 (1994)CrossRefGoogle Scholar
12. Marcaide, J. et al.: Astrophys. J. Lett. 424, L25 (1994)CrossRefGoogle Scholar
13. Marcaide, J.M. et al.: Astrophys. J. Lett. 486, L31 (1997)CrossRefGoogle Scholar
14. Mioduszewski, A.J., Dwarkadas, V.V., Bail, L.: Astrophys. J. 562, 869 (2001)CrossRefGoogle Scholar
15. Montes, M.J., Weiler, K.W., Panagia, N.: Astrophys. J. 488, 792 (1997)CrossRefGoogle Scholar
16. Pérez-Torres, M.A., Alberdi, A., Marcaide, J.M.: Astron. Astrophys. 374, 997 (2001)CrossRefGoogle Scholar
17. Pérez-Torres, M.A., Alberdi, A., Marcaide, J.M.: Astron. Astrophys., 394, 71 (2002)Google Scholar
18. Pooley, G.G., Green, D.A.: Mon. Not. R. Astron. Soc. 264, 17P (1993)CrossRefGoogle Scholar
19. Readhead, A.C.S.: Astrophys. J. 426, 51 (1994)CrossRefGoogle Scholar
20. Suzuki, T., Nomoto, K.: Astrophys. J. 455, 658 (1995)CrossRefGoogle Scholar
21. Swartz, D.A. et al.: Astrophys. J. 144, 213 (2003)CrossRefGoogle Scholar
22. Tanaka, Y.: IAUC 5753 (1993)CrossRefGoogle Scholar
23. Uno, S. et al.: Astrophys. J. 565, 419 (2002)CrossRefGoogle Scholar
24. Van Dyk, S.D., Weiler, K.W., Sramek, R.A., Rupen, M.P., Panagia, N.: Astrophys. J. Lett. 432, L115 (1994)CrossRefGoogle Scholar
25. Weiler, K.W. et al.: Astrophys. J. 301, 790 (1986)CrossRefGoogle Scholar
26. Weiler, K.W., Panagia, N., Sramek, R.A.: Astrophys. J. 364, 611 (1990)CrossRefGoogle Scholar
27. Weiler, K.W., Panagia, N., Montes, M.J., Sramek, R.A.: Ann. Rev. Astron. Astrophys. 40, 387 (2002)CrossRefGoogle Scholar
28. Zimmermann, H.-U., Lewin, W., Magnier, E., et al.: IAUC 5748 (1993)Google Scholar
29. Zimmermann, H.-U., Lewin, W., Predehl, P., et al.: Nature 367, 621 (1994)CrossRefGoogle Scholar
30. Zimmermann, H.-U., Aschenbach, B.: Astron. Astrophys. 406, 969 (2003)CrossRefGoogle Scholar