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Astrophysics
Article . 1987 . Peer-reviewed
License: Springer TDM
Data sources: Crossref
https://dx.doi.org/10.1007/bf0...
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Infrared photometry of FG Sge

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1987 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics, volume 25, pages 616-620 (issn: 0571-7132, eissn: 1573-8191, Copyright policy )
Authors: O. G. Taranova;

doi: 10.1007/bf01011223

Infrared photometry of FG Sge

Abstract

The results of UBVRJHKLM photometry of FG Sge made during 1985 are discussed. It follows from analysis of the observations that the spectral class of FG Sge in 1985 corresponded to G(1 +/- 0.5)I; for r = 4.1 kpc, the radius of the star is 95R/sub circle/ and L = 8.9 x 10/sup 3/L/sub circle/

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selected citations
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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.
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