Numerical studies of the Vishniac instability in supernova remnants

Details Numerical studies of the Vishniac instability in supernova remnants Numerical studies of the Vishniac instability in supernova remnants

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sf2a.conf..453c&link_type=abstract

"SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: C. Charbonnel, F. Combes

Astronomy and Astrophysics

Astrophysics

Scientific paper

Vishniac instability has been theoretically studied in supernova remnants where it is supposed to explain the fragmentation of the interstellar medium. However its role is not fully demonstrated in these astrophysical objects. Numerical simulations with the HYDRO-MUSCL hydrodynamic code has been realised to simulate this instability in order to compare the numerical growth rate with the Vishniac analytical solution.

Affiliated with

Also associated with

No associations

Rating

Numerical studies of the Vishniac instability in supernova remnants does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Numerical studies of the Vishniac instability in supernova remnants, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical studies of the Vishniac instability in supernova remnants will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1287862