Active Be stars

P. K. Barker

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Publications of the Astronomical Society of the Pacific

Article . 1983 . Peer-reviewed

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https://dx.doi.org/10.1086/131...

Article

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Active Be stars

descriptionPublicationkeyboard_double_arrow_right Article 01 Dec 1983 English Publisher:IOP PublishingJournal:Publications of the Astronomical Society of the Pacific, volume 95, page 996 (issn: 0004-6280, eissn: 1538-3873,

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Authors: P. K. Barker;

doi: 10.1086/131280

Active Be stars

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Abstract

Intensifier director scanner H-alpha profiles are presented of the bright northern Be stars, which have recently developed significant emission line variability. These stars are candidates for intensive spectroscopic, photometric, and polarimetric observations during the current season.

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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).	8
	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.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Top 10%
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average