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Astrophysics and Space Science
Article . 1990 . Peer-reviewed
License: Springer TDM
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https://dx.doi.org/10.1007/bf0...
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https://dx.doi.org/10.1007/bf0...
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Asymmetric winds in be stars

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1990 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 163, pages 49-58 (issn: 0004-640X, eissn: 1572-946X, Copyright policy )
Authors: F. X. De Araujo; J. A. de Freitas Pacheco;

doi: 10.1007/bf00639977

Asymmetric winds in be stars

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.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
1
Average
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