Hydrodynamical models of clumping beyond 50 stellar radii

Details Hydrodynamical models of clumping beyond 50 stellar radii Hydrodynamical models of clumping beyond 50 stellar radii

2007-11-13

arxiv.org/abs/0711.1939v1

Astronomy and Astrophysics

Astrophysics

International Workshop on clumping in Hot-Star Winds, June 2007, Potsdam, Germany. (3 pages, 2 figures)

Scientific paper

We present one-dimensional, time-dependent models of the clumps generated by
the line-deshadowing instability. In order to follow the clumps out to
distances of more than 1000 stellar radii, we use an efficient moving-box
technique. We show that, within the approximations, the wind can remain clumped
well into the formation region of the radio continuum.

Affiliated with

Also associated with

No associations

Rating

Hydrodynamical models of clumping beyond 50 stellar radii 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 Hydrodynamical models of clumping beyond 50 stellar radii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hydrodynamical models of clumping beyond 50 stellar radii will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-270341