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The Astrophysical Journal
Article . 1992 . Peer-reviewed
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https://dx.doi.org/10.1086/186...
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The peculiar fast nova Herculis 1991

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1992 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 384, page L41 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: Charles E. Woodward; R. D. Gehrz; Terry J. Jones; G. F. Lawrence;

doi: 10.1086/186258

The peculiar fast nova Herculis 1991

Abstract

Unlike previously observed fast novae, the temporal evolution of Nova Her 1991 is similar to slower, dusty novae in which the appearance of thermal infrared emission from condensing dust was coincident with a transition in the visible light curve. However, the total luminosity radiated by Nova Her 1991 in the infrared was only ∼5% of the outburst luminosity. It is suggested that the dust formed in the shell of Nova Her 1991 consisted of dense clumps with a covering factor of less than unity, and that one of these clumps formed along the line of sight to the central star

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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!
30
Average
Top 10%
Top 10%
gold