Non-LTE line formation in early B and late O stars. III - Singly ionized carbon

Details Non-LTE line formation in early B and late O stars. III - Singly ionized carbon Non-LTE line formation in early B and late O stars. III - Singly ionized carbon

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...202..153e&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 202, no. 1-2, Aug. 1988, p. 153-158.

Astronomy and Astrophysics

Astrophysics

74

B Stars, Carbon, Line Spectra, Nonequilibrium Thermodynamics, O Stars, Stellar Atmospheres, Stellar Spectra, Abundance, Early Stars, Late Stars, Stellar Composition, Stellar Temperature

Scientific paper

Extensive non-LTE calculations for C II are presented. Special emphasis is placed on the λ4267 Å line and it is demonstrated that the current results give the observed strength of this line with normal carbon abundance. A grid of equivalent widths is tabulated for lineblanketed LTE model atmospheres at early B and late O star temperatures.

Affiliated with

Also associated with

No associations

Rating

Non-LTE line formation in early B and late O stars. III - Singly ionized carbon 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 line formation in early B and late O stars. III - Singly ionized carbon, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-LTE line formation in early B and late O stars. III - Singly ionized carbon will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1693057