Non-LTE analysis of carbon lines in the spectra of hot stars

Details Non-LTE analysis of carbon lines in the spectra of hot stars Non-LTE analysis of carbon lines in the spectra of hot stars

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..917s&link_type=abstract

Astronomicheskii Zhurnal, Vol. 60, p.917

Astronomy and Astrophysics

Astronomy

5

Scientific paper

A determination of theoretical intensities of the C III - C IV lines in spectra of O - B stars has been carried out on the basis of a detailed solution of the coupled statistical-equilibrium and transfer equations for a multi-line, multi-level, and multi-ion ensemble. Also the comparison of these data with the observed ones is given. It is found that an analysis of subordinate lines of these ions gives the carbon abundance not much different from the normal one. The resonance lines show a large difference between theoretical and observed values which is believed to be a result of stellar wind effects.

Affiliated with

Also associated with

No associations

Rating

Non-LTE analysis of carbon lines in the spectra of hot 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 Non-LTE analysis of carbon lines in the spectra of hot stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-LTE analysis of carbon lines in the spectra of hot stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1192823