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arXiv · 1201.5223

Analytical and Monte Carlo results for the surface-brightness diameter relationship in supernova remnants

L. Zaninetti
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Abstract

The surface brightness diameter relationship for supernovae remnants (SNRs) is explained by adopting a model of direct conversion of the flux of kinetic energy into synchrotron luminosity. Two laws of motion are adopted, a power law model for the radius-time relationship, and a model which uses the thin layer approximation. The fluctuations on the log-log surface diameter relationship are modeled by a Monte Carlo simulation. In this model a new probability density function for the density as function of the galactic height is introduced.

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L. Zaninetti. 2012-01-25. Analytical and Monte Carlo results for the surface-brightness diameter relationship in supernova remnants. https://doi.org/10.1088/0004-637x/746/1/56

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