Asymmetric winds in be stars
DOI: 10.1007/BF00639977
Bibcode: 1990Ap&SS.163...49D
de Freitas Pacheco, J. A.; de Araujo, F. X.
Brazil
Abstract
The CIV and SiIV resonance doublets of 43 Be stars are investigated. Measurements of the equivalent widths seem to reveal a correlation between the strenght of the lines and the projected rotational velocity (v sini). it is discussed whether this result indicate that the wind region is not spherically symmetric.
1990
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Astrophysics and Space Science
IUE
1