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Radio Monitoring of Supernova 2001ig: The First Year

Published online by Cambridge University Press:  19 September 2016

Stuart D. Ryder ,
Elaine Sadler ,
Ravi Subrahmanyan ,
Kurt W. Weiler ,
Nino Panagia  and
Christopher Stockdale
Stuart D. Ryder
Affiliation:
Anglo-Australian Observatory, P.O. Box 296, Epping, NSW 1710, Australia; sdr@aaoepp.aao.gov.au
Elaine Sadler
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia; ems@physics.usyd.edu.au
Ravi Subrahmanyan
Affiliation:
Australia Telescope National Facility, CSIRO, Locked Bag 194, Narrabri, NSW 2390, Australia; Ravi.Subrahmanyan@csiro.au
Kurt W. Weiler
Affiliation:
Naval Research Laboratory, Code 7213 Washington, DC 20375-5320, USA; Kurt.Weiler@nrl.navy.mil
Nino Panagia
Affiliation:
ESA/Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA; panagia@stsci.edu
Christopher Stockdale
Affiliation:
Naval Research Laboratory, Code 7213 Washington, DC 20375-5320, USA; Kurt.Weiler@nrl.navy.mil Physics Dept., Marquette University, P.O. Box 1881 Milwaukee, WI 53201, USA; Christopher.Stockdale@marquette.edu

Summary

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Supernova 2001ig in NGC 7424 has been observed with the Australia Telescope Compact Array at ~2 week intervals since its discovery, making this the best-studied Type IIb radio supernova since SN 1993J. We present radio light curves for frequencies from 1.4 to 20 GHz, and preliminary attempts to model the observed behavior. Since peaking in radio luminosity at 8.6 and 4.8 GHz some 1-2 months after the explosion, SN 2001ig has on at least two occasions deviated significantly from a smooth decline, indicative of interaction with a dense circumstellar medium and possibly of periodic progenitor mass-loss.

Information

Type
Part I Supernovae: Individual
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 123 - 128
Copyright
Copyright © Springer-Verlag 2005

References

1. Chevalier, R.: Astrophys. J. 259, 302 (1982)Google Scholar
2. Clocchiatti, A., Prieto, J.L.: IAUC 7781 (2001)Google Scholar
3. Clocchiatti, A.: IAUC 7793 (2002)Google Scholar
4. Evans, R.O.: IAUC 7772 (2001)Google Scholar
5. Filippenko, A.V.: Astron. J. 96, 1941 (1988)Google Scholar
6. Filippenko, A.V., Chornock, R.: IAUC 7988 (2002)Google Scholar
7. Iben, I., Renzini, A.: Ann. Rev. Astron. Astrophys. 21, 271 (1983)Google Scholar
8. Matheson, T., Jha, S.: IAUC7772 (2001)Google Scholar
9. Monnier, J.D., Tuthill, P.G., Danchi, W.C.: Astrophys. J. Lett. 525, L97 (1999)Google Scholar
10. Montes, M.J. et al.: Astrophys. J. 532, 1124 (2000)Google Scholar
11. Ryder, S.D. et al.: Astrophys. J. 416, 167 (1993)Google Scholar
12. Ryder, S.D., Kranz, K., Sadler, E., Subrahmanyan, R.: IAUC 7777 (2001)Google Scholar
13. Schlegel, E.M. et al.: Astron. J. 118, 2689 (1999)Google Scholar
14. Schlegel, E.M., Ryder, S.D.: IAUC 7913 (2002)Google Scholar
15. Schwarz, D.H., Pringle, J.E.: Mon. Not. R. Astron. Soc. 282, 1018 (1996)Google Scholar
16. Staveley-Smith, L. et al.: Nature 355, 147 (1992)Google Scholar
17. Tully, R.B.: In: Nearby Galaxies Catalog (Cambridge Univ. Press: Cambridge, 1988)Google Scholar
18. Tuthill, P.G., Monnier, J.D., Danchi, W.C.: Nature 398, 487 (1999)Google Scholar
19. Van Dyk, S.: In: these ProceedingsGoogle Scholar
20. Weiler, K.W., Van Dyk, S.D., Pringle, J.E., Panagia, N.: Astrophys. J. 399, 672 (1992)Google Scholar
21. Weiler, K.W., Panagia, N., Montes, M., Sramek, R.A.: Ann. Rev. Astron. Astrophys. 40, 387 (2002)Google Scholar
22. Wieringa, M.H., Kulkami, S.R., Frail, D.A.: Astron. Astrophys. Suppl. 138, 467 (1999)Google Scholar