Fe II Line Widths as Tracers for the Geometry of Be Star Envelopes
- 1 January 1994
- book chapter
- Published by Springer Nature
Abstract
No abstract availableKeywords
This publication has 2 references indexed in Scilit:
- Stellarv sini and optical emission line widths in Be starsAstrophysics and Space Science, 1989
- Spectral types and rotational velocities of the brighter Be stars and A-F type shell starsThe Astrophysical Journal Supplement Series, 1982