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Modeling the Radio and X-ray Emission of SN 1993J and SN 2002ap
| Content Provider | Scilit |
|---|---|
| Author | Fransson, Claes Björnsson, Claes-Ingvar |
| Copyright Year | 2005 |
| Description | Summary: 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. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/3F81B129CACA0F3D9FFAE2D56754FEBF/S0252921100009003a.pdf/div-class-title-modeling-the-radio-and-x-ray-emission-of-sn-1993j-and-sn-2002ap-div.pdf |
| Ending Page | 69 |
| Page Count | 11 |
| Starting Page | 59 |
| ISSN | 02529211 |
| DOI | 10.1017/s0252921100009003 |
| Journal | International Astronomical Union Colloquium |
| Volume Number | 192 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2005-01-01 |
| Access Restriction | Open |
| Subject Keyword | International Astronomical Union Colloquium Astronomy and Astrophysics Sn 2002ap 1993j and Sn Radio and X Modeling the Radio |
| Content Type | Text |
| Resource Type | Article |
