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arXiv.org e-Print Archive
Preprint . 2014
Data sources: arXiv.org e-Print Archive
https://dx.doi.org/10.48550/ar...
Article . 2014
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Rotation of White Dwarf Stars

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Jan 2014Embargo end date: 01 Jan 2014Publisher:arXiv
Authors: Kawaler, Steven D.;

doi: 10.48550/arxiv.1410.6934

arXiv: http://arxiv.org/abs/1410.6934

Rotation of White Dwarf Stars

Abstract

I discuss and consider the status of observational determinations of the rotation velocities of white dwarf stars via asteroseismology and spectroscopy. While these observations have important implications on our understanding of the angular momentum evolution of stars in their late stages of evolution, more direct methods are sorely needed to disentangle ambiguities.

5 pages, 1, figure, to appear in the proceedings of the 19th European White Dwarf Workshop held August 11-15, 2014 in Montreal, Canada

Related Organizations
Keywords

Astrophysics - Solar and Stellar Astrophysics, FOS: Physical sciences, Solar and Stellar Astrophysics (astro-ph.SR)

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citations
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!
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Average
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Average
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