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The Astrophysical Journal
Article . 2002 . Peer-reviewed
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arXiv.org e-Print Archive
Preprint . 2002
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Article . 2016
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https://dx.doi.org/10.48550/ar...
Article . 2002
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On the Population of Wind-accreting Neutron Stars in the Galaxy

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 20 May 2002Embargo end date: 01 Mar 2002 United Kingdom Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 571, pages L37-L40 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: Pfahl, E; Rappaport, S; Podsiadlowski, P;

doi: 10.1086/341197 , 10.48550/arxiv.astro-ph/0203266

arXiv: astro-ph/0203266

On the Population of Wind-accreting Neutron Stars in the Galaxy

Abstract

We explore the possibility that neutron stars accreting from the winds of main-sequence stellar companions account for a significant fraction of low-luminosity, hard X-ray sources (L_X

submitted to ApJ Letters

Country
United Kingdom
Related Organizations
Keywords

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

  • BIP!
    Impact byBIP!
    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).
    		 82
    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.
    		 Top 10%
    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.
    		 Top 10%
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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!
82
Top 10%
Top 10%
Top 10%
Green
gold
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