Gravitational wave signals from the first massive black hole seeds

ABSTRACT. Recent numerical simulations reveal that the isothermal collapse of pristine gas in atomic cooling haloes may result in stellar binaries of supermass

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Bibliographic Details
Main Authors: Hartwig, Tilman (Author) , Agarwal, Bhaskar (Author) , Regan, John A. (Author)
Format: Article (Journal)
Language:English
Published: 24 May 2018
In: Monthly notices of the Royal Astronomical Society. Letters
Year: 2018, Volume: 479, Issue: 1, Pages: L23-L27
ISSN:1745-3933
DOI:10.1093/mnrasl/sly091
Online Access:Verlag, Volltext: https://doi.org/10.1093/mnrasl/sly091
Verlag: https://academic.oup.com/mnrasl/article/479/1/L23/5003389
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Author Notes:Tilman Hartwig, Bhaskar Agarwal and John A. Regan
Description
Summary:ABSTRACT. Recent numerical simulations reveal that the isothermal collapse of pristine gas in atomic cooling haloes may result in stellar binaries of supermass
Item Description:Gesehen am 16.10.2019
Physical Description:Online Resource
ISSN:1745-3933
DOI:10.1093/mnrasl/sly091