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

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

2012-01-25

arxiv.org/abs/1201.5223v1

published on Apj 746 , 56 (2012)

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

24 pages 8 figures

Scientific paper

10.1088/0004-637X/746/1/56

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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