Non-LTE line formation in early B and late O stars. IV - Singly ionized nitrogen

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

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...209..244b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 209, no. 1-2, Jan. 1989, p. 244-254.

Astronomy and Astrophysics

Astrophysics

72

B Stars, Line Spectra, Nitrogen Ions, Nonequilibrium Thermodynamics, O Stars, Stellar Spectra, Oxygen Ions, Photoionization, Stellar Atmospheres, Stellar Models

Scientific paper

An extensive model atom for a non-LTE line formation determination for N II is discussed. Based on B star model atmospheres, a grid of equivalent widths for over 35 N-II lines in the wavelength region from 4000-5000 A has been obtained in both non-LTE and LTE. An abundance determination for nitrogen in Tau Sco using the model atom demonstrates that the non-LTE analysis produces reliable results.

Affiliated with

Also associated with

No associations

Rating

Non-LTE line formation in early B and late O stars. IV - Singly ionized nitrogen 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. IV - Singly ionized nitrogen, 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. IV - Singly ionized nitrogen will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-824811