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The Astrophysical Journal
Article . 1972 . Peer-reviewed
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https://dx.doi.org/10.1086/151...
Article
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https://dx.doi.org/10.1086/151...
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Wolf-Rayet Stars in M33.

descriptionPublicationkeyboard_double_arrow_right Article 01 Mar 1972 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 172, page 577 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: James D. Wray; George J. Corso;

doi: 10.1086/151375

Wolf-Rayet Stars in M33.

Abstract

Twenty-five objects in M33 have been identified as Wolf-Rayet stars on the basis of narrow-band interference-filter photography. Spectra of two of the objects obtained by Lynds have been interpreted as WC5 or 6 +OB. Apparent blue continuum magnitudes range from +17.6 to the plate limit at +19.8 yielding absolute magnitudes in reasonable agreement with the magnitudes of Wolf-Rayet stars in the Magellanic Clouds.

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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!
21
Average
Top 10%
Average
gold