Large scale structures and synchrotron emission
I. Asymmetric supernova remnants
Received 8 July 1997 / Accepted 10 February 2000
In order to attack the problem of asymmetric shapes of the observed Supernova Remnants, a numerical technique is developed that divides the sphere into many sectors. Using this numerical method, some of the observed features of the supernova remnants, like a barrel shape or multi-ring shape can be reproduced.
Key words: ISM: bubbles ISM: supernova remnants radio continuum: stars
Send offprint requests to: L. Zaninetti
© European Southern Observatory (ESO) 2000
Online publication: April 17, 2000