Shocks in Multicomponent Astrophysical Media

Details Shocks in Multicomponent Astrophysical Media Shocks in Multicomponent Astrophysical Media

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..401..177h&link_type=abstract

RS Ophiuchi (2006) and the Recurrent Nova Phenomenon ASP Conference Series, Vol. 401, proceedings of the conference held 12-14 J

Astronomy and Astrophysics

Astrophysics

Scientific paper

Many diffuse astrophysical media consist of multiple components, and their multicomponent natures affect the evolution of shocks in them. The focus here is on three problems concerning multicomponent models of media containing shocks. The subject of the first is the cosmic ray modification of shocks in supernova remnants and recently begun efforts to model observed shocks in the Tycho and Cygnus Loop remnants. The next involves shocks in the central 25 kpc of the Perseus cluster of galaxies which may contain an AGN-driven fountain flow in which multiple phase changes occur. The final one concerns multifluid models of shocks in magnetized, dense, dusty star forming regions. The exposition is mostly about work still in progress or that has not even fully begun.

Affiliated with

Also associated with

No associations

Rating

Shocks in Multicomponent Astrophysical Media 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 Shocks in Multicomponent Astrophysical Media, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Shocks in Multicomponent Astrophysical Media will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-962127