Chandra, P. ; Ray, A. ; Sutaria, F. (2004) X-ray and radio prompt emission from a hypernova SN 2002ap Nuclear Physics B - Proceedings Supplements, 132 . pp. 308-311. ISSN 09205632
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Official URL: http://doi.org/10.1016/j.nuclphysbps.2004.04.054
Related URL: http://dx.doi.org/10.1016/j.nuclphysbps.2004.04.054
Abstract
Here we report on combined X-ray and radio observations of SN 2002ap with XMM-Newton ToO observation and GMRT observations aided with VLA published results. In deriving the X-ray flux of SN 2002ap we account for the contribution of a nearby source, found to be present in the pre-SN explosion images obtained with Chandra observatory. We also derive upper limits on the mass loss rate from X-ray and radio data. We suggest that the prompt X-ray emission is non-thermal in nature and due to the repeated compton boosting of optical photons. We also compare the SN's early radiospheric properties with two other SNe at the same epoch.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to Elsevier B.V |
| ID Code: | 125954 |
| Deposited On: | 17 Oct 2022 09:03 |
| Last Modified: | 17 Oct 2022 09:03 |
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