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Monthly Notices of the Royal Astronomical Society
Article . 2022 . Peer-reviewed
License: OUP Standard Publication Reuse
Data sources: Crossref
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arXiv.org e-Print Archive
Preprint . 2021
Data sources: arXiv.org e-Print Archive
https://dx.doi.org/10.48550/ar...
Article . 2021
License: CC BY
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Subsonic wind accretion

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 25 Mar 2022Embargo end date: 01 Jan 2021 English Publisher:Oxford University Press (OUP)Journal:Monthly Notices of the Royal Astronomical Society, volume 512, pages 2,154-2,156 (issn: 0035-8711, eissn: 1365-2966, Copyright policy )
Authors: Gruzinov, Andrei;

doi: 10.1093/mnras/stac513 , 10.48550/arxiv.2112.11221

arXiv: 2112.11221

Subsonic wind accretion

Abstract

ABSTRACT The rate of subsonic wind accretion (accretion on a point Newtonian mass moving through uniform gas) is shown to be independent of the wind velocity and equal to the spherical Bondi rate – for the adiabatic index equal to 5/3. A (very accurate) numerical calculation of the accretion flow, confirming this result, is also presented.

Related Organizations
Keywords

High Energy Astrophysical Phenomena (astro-ph.HE), FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena

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    selected citations
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    		 3
    popularity
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    		 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).
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    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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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!
3
Top 10%
Average
Average
Green
gold