Are the Supernova Remnants of the Large Magellanic Cloud in the Adiabatic Phase

Details Are the Supernova Remnants of the Large Magellanic Cloud in the Adiabatic Phase Are the Supernova Remnants of the Large Magellanic Cloud in the Adiabatic Phase

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..315f&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

2

Scientific paper

The catalog of LMC supernova remnants (SNRs) observed by Einstein in the
0.15 - 4.5 keV X-ray band is analyzed. It is shown that the X-ray
surface brightness as a function of linear radius and the cumulative
number-radius relation can be explained assuming that the SNRs in the
LMC are in the adiabatic phase.

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