Dynamics and Radiation of Young Type-Ia Supernova Remnants: Important Physical Processes

Details Dynamics and Radiation of Young Type-Ia Supernova Remnants: Important Physical Processes Dynamics and Radiation of Young Type-Ia Supernova Remnants: Important Physical Processes

2005-02-01

arxiv.org/abs/astro-ph/0502026v2

Astron.Lett. 30 (2004) 737-750

Astronomy and Astrophysics

Astrophysics

19 pages, 8 figures

Scientific paper

10.1134/1.1819492

We examine and analyze the physical processes that should be taken into account when modeling young type-Ia SNRs, with ages of several hundred years. It is shown, that energy losses in the metal-rich ejecta can be essential for remnants already at this stage of evolution. The influence of electron thermal conduction and the rate of the energy exchange between electrons and ions on the temperature distribution and the X-radiation from such remnants is studied. The data for Tycho SNR from the XMM-Newton X-ray telescope have been employed for the comparison of calculations with observations.

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