No CrossRef data available.
Article contents
Circumstellar interaction in Type IIn supernovae
Published online by Cambridge University Press: 29 January 2014
Abstract
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.
Type IIn supernovae have bright optical emission and high bolometric luminosities. Due to their high mass loss, their are expected to have dense circumstellar interaction, thus produce bright radio and X-ray emission. We aim to carry out systematic study to understand their circumstellar interaction, mass loss properties. Here, I provide specific examples of two Type IIn supernovae, 2006jd and 2010jl.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 135 - 143
- Copyright
- Copyright © International Astronomical Union 2014
References
Chevalier, R. A. & Fransson, C. 2003, in: Weiler, K. (eds.), Supernovae and Gamma-Ray Bursters: Lecture Notes in Physics (Berlin: Springer), vol. 598, p. 171Google Scholar
Kallman, T. R., Palmeri, P., Bautista, M. A., Mendoza, C., & Krolik, J. H. 2004, ApJS, 155, 675Google Scholar
Patat, F., Taubenberger, S., Benetti, S., Pastorello, A., & Harutyunyan, A. 2011, A&A, 527, L6Google Scholar
van Dyk, S. D., Weiler, K. W., Sramek, R. A., & Panagia, N. 1993, ApJ, 419, L69CrossRefGoogle Scholar
You have
Access