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On the kinematics of the variable DA stars.

descriptionPublicationkeyboard_double_arrow_right Article 01 Apr 1978 English Publisher:IOP PublishingJournal:Publications of the Astronomical Society of the Pacific, volume 90, page 154 (issn: 0004-6280, eissn: 1538-3873, Copyright policy )
Authors: E. M. Sion; O. L. Lupie; K. N. Young;

doi: 10.1086/130298

On the kinematics of the variable DA stars.

Abstract

We examine the kinematics of the known variable DA white dwarfs relative to a sample of observed nonvariable DA white dwarfs in the same color range. The variable DA stars do not form a kinematically distinct group relative to the nonvariable stars. Possible implications based upon the kinematics are briefly discussed. Key words: white dwarfs-pulsations-kinematics

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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!
2
Average
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