The Advective-Acoustic Instability in Numerical Simulations of Astrophysical Flows

Details The Advective-Acoustic Instability in Numerical Simulations of Astrophysical Flows The Advective-Acoustic Instability in Numerical Simulations of Astrophysical Flows

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..385...85f&link_type=abstract

Numerical Modeling of Space Plasma Flows: Astronum 2007 ASP Conference Series, Vol. 385, proceedings of the conference held 10-1

Astronomy and Astrophysics

Astrophysics

Scientific paper

The advective-acoustic instability has been introduced in astrophysics to explain the instability of Bondi--Hoyle accretion flows. Its effects seem to be most promising in the problem of core collapse supernovae, where it contributes to revive the stalled shock during the first second of the explosion, leading to an asymmetric explosion, a pulsar kick and spin up. I review our understanding of this instability, and comment on its treatment in numerical simulations.

Affiliated with

Also associated with

No associations

Rating

The Advective-Acoustic Instability in Numerical Simulations of Astrophysical Flows 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 The Advective-Acoustic Instability in Numerical Simulations of Astrophysical Flows, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Advective-Acoustic Instability in Numerical Simulations of Astrophysical Flows will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1198675