Line shapes of rotating stars with application to Alpha Lyrae

Details Line shapes of rotating stars with application to Alpha Lyrae Line shapes of rotating stars with application to Alpha Lyrae

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...384..284e&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 384, Jan. 1, 1992, p. 284-291.

Astronomy and Astrophysics

Astrophysics

8

Line Spectra, Spectral Line Width, Stellar Rotation, Stellar Spectra, Stellar Spectrophotometry

Scientific paper

Profiles of weak and medium strong lines in the high-resolution spectrum
of Vega can in principle be understood by the center-to-limb variation
of their equivalent widths, predicted by a standard model atmosphere.
Finer details may require a different model structure depending on the
latitude of the rotating star, and perhaps differential rotation.

Affiliated with

Also associated with

No associations

Rating

Line shapes of rotating stars with application to Alpha Lyrae 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 shapes of rotating stars with application to Alpha Lyrae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Line shapes of rotating stars with application to Alpha Lyrae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-934648