Line-blanketed model atmospheres for WR stars

Details Line-blanketed model atmospheres for WR stars Line-blanketed model atmospheres for WR stars

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...387..244g&link_type=abstract

Astronomy and Astrophysics, v.387, p.244-257 (2002)

Astronomy and Astrophysics

Astrophysics

64

Stars: Wolf-Rayet, Stars: Atmospheres, Stars: Abundances, Stars: Early-Type, Stars: Mass Loss, Stars: Individual: Wr 111

Scientific paper

We describe the treatment of iron group line-blanketing in non-LTE model atmospheres for WR stars. As an example, a blanketed model for the early-type WC star WR 111 is compared to its un-blanketed counterpart. Blanketing affects the ionization structure and the emergent flux distribution of our models. The radiation pressure, as computed within our models, falls short by only a factor of two to provide the mechanical power of the WR wind.

Affiliated with

Also associated with

No associations

Rating

Line-blanketed model atmospheres for WR stars 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 Line-blanketed model atmospheres for WR stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Line-blanketed model atmospheres for WR stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1716890