Stellarv sini and optical emission line widths in Be stars
- 1 January 1989
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 161 (1) , 61-73
- https://doi.org/10.1007/bf00653238
Abstract
No abstract availableKeywords
This publication has 5 references indexed in Scilit:
- Spectral types and rotational velocities of the brighter Be stars and A-F type shell starsThe Astrophysical Journal Supplement Series, 1982
- Further studies of stellar rotation from Copernicus satellite dataPublications of the Astronomical Society of the Pacific, 1979
- Be star models : observable effects of model parameters.The Astrophysical Journal Supplement Series, 1978
- Profiles of Emission Lines in be StarsThe Astrophysical Journal, 1972
- On the Origin of Bright Lines in Spectra of Stars of Class BThe Astrophysical Journal, 1931