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The Astrophysical Journal
Article
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arXiv.org e-Print Archive
Preprint . 1996
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The Astrophysical Journal
Article . 1996 . Peer-reviewed
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https://dx.doi.org/10.48550/ar...
Article . 1996
License: arXiv Non-Exclusive Distribution
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https://dx.doi.org/10.1086/310...
Article
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https://dx.doi.org/10.1086/310...
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“Chain” Galaxies Are Edge-On Low Surface Brightness Galaxies

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jul 1996Embargo end date: 01 Jan 1996Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 465, pages L9-L13 (issn: 0004-637X, Copyright policy )
Authors: Dalcanton, J. J.; Shectman, S. A.;

doi: 10.1086/310124 , 10.48550/arxiv.astro-ph/9604157

arXiv: astro-ph/9604157

“Chain” Galaxies Are Edge-On Low Surface Brightness Galaxies

Abstract

Deep HST WFPC2 images have revealed a population of very narrow blue galaxies which Cowie et al. (1996) have interpreted as being a new morphological class of intrinsically linear star forming galaxies at $z=0.5-3$. We show that the same population exists in large numbers at low redshifts (z=0.03) and are actually the edge-on manifestation of low surface brightness disk galaxies.

18 pages + 3 pages of figures. Uuencoded, gzipped, tar file of 1 latex file, 5 figures, and 2 latex style files. To appear in the Astrophysical Journal Letters

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Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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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!
34
Top 10%
Top 10%
Top 10%
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