Radiative steady-state colliding stellar wind models: are they correct?

Details Radiative steady-state colliding stellar wind models: are they correct? Radiative steady-state colliding stellar wind models: are they correct?

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.298.1021m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 298, Issue 4, pp. 1021-1029.

Astronomy and Astrophysics

Astronomy

26

Hydrodynamics, Instabilities, Shock Waves, Binaries: General

Scientific paper

The properties of radiative steady-state colliding stellar winds in binary systems are studied. It is shown that the presence of a singularity at the stagnation point has a major influence on the structure of these flows. This problem is of great importance if their stability properties are considered. None of the existing models treats this mathematical problem properly, and special efforts must be undertaken in the future in order to come to a firm conclusion about the physical nature of possible instabilities. At the moment, neither numerical nor analytical models can be considered to be of acceptable accuracy in the case of highly radiative steady-state colliding stellar winds.

Affiliated with

Also associated with

No associations

Rating

Radiative steady-state colliding stellar wind models: are they correct? 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 Radiative steady-state colliding stellar wind models: are they correct?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiative steady-state colliding stellar wind models: are they correct? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1535589