Energetics of Supernova Remnants

Details Energetics of Supernova Remnants Energetics of Supernova Remnants

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001stin...0178199c&link_type=abstract

Technical Report, Illinois Univ. United States

Physics

Supernova Remnants, Wavelengths, Magellanic Clouds, Rosat Mission, Ambience, Energy Distribution, Data Processing, Thermodynamic Properties

Scientific paper

We proposed to carry out a multi-wavelength analysis of SNR energetics for a large number of Large Magellanic Cloud (LMC) SNRs in different stages of evolution and with different ambient interstellar environments. This analysis will provide insight as to how the energy of a SNR is partitioned in different forms, such as thermal, kinetic, and magnetic energies. The variety of SNR environments will allow us to evaluate the effects of local ISM conditions in the energy distributions in the SNRs, and how some of the energy is transferred to the surrounding ISM. The main dataset used in this study is from the ROSAT archive, and the secondary dataset is from the ASCA archive.

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