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Radio-loudness in black hole transients: evidence for an inclination effect

Abstract:

Accreting stellar-mass black holes appear to populate two branches in a radio:X-ray luminosity plane. We have investigated the X-ray variability properties of a large number of black hole low-mass X-ray binaries, with the aim of unveiling the physical reasons underlying the radio-loud/radio-quiet nature of these sources, in the context of the known accretion–ejection connection. A reconsideration of the available radio and X-ray data from a sample of black hole X-ray binaries confirms that be...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's Version

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Publisher copy:
10.1093/mnras/sty1440

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Astrophysics
ORCID:
0000-0002-6154-5843
Casella, P More by this author
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Astrophysics
Oxford college:
Brasenose College
Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
478
Issue:
4
Pages:
5159–5173
Publication date:
2018-06-02
Acceptance date:
2018-05-30
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:857841
URN:
uri:da17f93e-e519-4cb5-9289-da8074fae620
UUID:
uuid:da17f93e-e519-4cb5-9289-da8074fae620
Local pid:
pubs:857841

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