Winds

Details Winds Winds

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aspc...40..620m&link_type=abstract

In: Inside the stars; Proceedings of the 137th IAU Colloquium, Univ. of Vienna, Austria, Apr. 13-18, 1992 (A93-53126 23-90), p.

Statistics

Computation

1

Main Sequence Stars, Stellar Interiors, Stellar Mass Ejection, Stellar Winds, Computational Astrophysics, Massive Stars, Stellar Atmospheres, Stellar Composition, Stellar Evolution, Stellar Rotation, Stellar Structure

Scientific paper

It is by now well known that most main sequence stars continuously lose mass as a consequence of the winds they emit. In addition to affecting the thermal and dynamical state of the stellar atmosphere, such mass loss can also induce changes in the interiors of stars. In the present review, we consider a few of the ways in which sustained, wind-like mass loss can alter the physical state of main sequence stellar interiors by examining the differences in internal structure, composition, and rotation between mass-losing and conservatively evolving stars.

Affiliated with

Also associated with

No associations

Rating

Winds 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 Winds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Winds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1779022