Collisionless Slowing Down of Nova and Supernova Shells in Magnetized Interstellar Medium

Details Collisionless Slowing Down of Nova and Supernova Shells in Magnetized Interstellar Medium Collisionless Slowing Down of Nova and Supernova Shells in Magnetized Interstellar Medium

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap.....46..434o&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 46, Issue 4, p. 434-444 (2003).

Astronomy and Astrophysics

Astrophysics

4

Novae Stars - Supernovae Stars - Ism Magnetic Fields

Scientific paper

The collisionless interaction of an expanding plasma cloud with a magnetized background plasma is examined in the framework of a 3D kinetic-hydrodynamic model. The slowing down of a hydrogen cloud is studied for high Alfven-Mach numbers and magneto-laminar interaction parameters. A particle-in-cell method is used to study the dynamics of the magnetic field, plasma cloud, background plasma, and collisionless shock wave generated by the intense particle flux. A numerical simulation is consistent with the nonstationary interactions between the plasma shells formed during nova and supernova explosions and the interstellar plasma medium.

Affiliated with

Also associated with

No associations

Rating

Collisionless Slowing Down of Nova and Supernova Shells in Magnetized Interstellar Medium 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 Collisionless Slowing Down of Nova and Supernova Shells in Magnetized Interstellar Medium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Collisionless Slowing Down of Nova and Supernova Shells in Magnetized Interstellar Medium will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-912839