Colliding Winds in Binary Star Systems: Theory, Models

Details Colliding Winds in Binary Star Systems: Theory, Models Colliding Winds in Binary Star Systems: Theory, Models

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.260..243w&link_type=abstract

Astrophysics and Space Science, v. 260, Issue 1/2, p. 243-252 (1998).

Astronomy and Astrophysics

Astrophysics

18

Scientific paper

The properties of the interaction region of colliding winds in hot star binaries and evolved low mass binaries are discussed in the frame of 2D and 3D hydrodynamical numerical simulations. The emission of such systems and their nebulae, in particular in X-rays, is reviewed and new results regarding orbital line profile variations are presented. The connection between colliding winds, thin shell instabilities and structure formation is outlined.

Affiliated with

Also associated with

No associations

Rating

Colliding Winds in Binary Star Systems: Theory, Models 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 Colliding Winds in Binary Star Systems: Theory, Models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Colliding Winds in Binary Star Systems: Theory, Models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1719973