A fully blanketed early B star LTE model atmosphere using an opacity sampling technique

Details A fully blanketed early B star LTE model atmosphere using an opacity sampling technique A fully blanketed early B star LTE model atmosphere using an opacity sampling technique

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192..197p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, July 1980, p. 197-207. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

3

B Stars, Early Stars, Opacity, Stellar Atmospheres, Stellar Models, Thermodynamic Equilibrium, Absorption Spectra, Atmospheric Models, Stellar Spectra, Ultraviolet Spectra

Scientific paper

A fully blanketed LTE model of a stellar atmosphere with Te = 21,914 K, log g = 4 is presented. The model includes an explicit representation of the opacity due to the strongest lines, and uses a statistical opacity sampling technique to represent the weaker line opacity. The sampling technique is subjected to several tests and the model is compared with an atmosphere calculated using the line-distribution function method. The limitations of the distribution function method and the particular opacity sampling method used here are discussed in the light of the results obtained.

Affiliated with

Also associated with

No associations

Rating

A fully blanketed early B star LTE model atmosphere using an opacity sampling technique 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 A fully blanketed early B star LTE model atmosphere using an opacity sampling technique, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A fully blanketed early B star LTE model atmosphere using an opacity sampling technique will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-804466