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Astrophysics and Space Science
Article . 1972 . Peer-reviewed
License: Springer TDM
Data sources: Crossref
https://dx.doi.org/10.1007/bf0...
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Stellar winds and mass loss of a rotating star

descriptionPublicationkeyboard_double_arrow_right Article 01 Sep 1972 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 18, pages 128-134 (issn: 0004-640X, eissn: 1572-946X, Copyright policy )
Authors: J. P. De Grève; C. De Loore; C. De Jager;

doi: 10.1007/bf00645286

Stellar winds and mass loss of a rotating star

Abstract

The mass loss to be expected from the corona of a rotating F2-star is calculated. The rotation is supposed to be rigid up to a certain distances, as if it were maintained by a strong magnetic field. Dependent on the values of the rotational velocity the mass loss can increase to 26–40% forvrot up to 200 km s−1.

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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!
5
Average
Average
Average
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