No evidence for a low-mass black hole in Swift J1753.5-0127

Bibcode
2016MNRAS.463.1314S
DOI
10.1093/mnras/stw2092
Shaw, A. W.; Charles, P. A.; Casares, J.; Hernández Santisteban, J. V.
Bibliographical reference

Monthly Notices of the Royal Astronomical Society, Volume 463, Issue 2, p.1314-1322

Advertised on:
12
2016
Journal
Monthly Notices of the Royal Astronomical Society
Number of authors
4
IAC number of authors
1
Citations
22
Refereed citations
22
Description
We present high-resolution, time-resolved optical spectroscopy of the black hole X-ray transient Swift J1753.5-0127. Our optical spectra do not show features that we can associate with the companion star. However we do observe broad, double-peaked emission lines, typical of an accretion disc. We show that the mass of the compact object is likely >7.4 ± 1.2 M⊙, much higher than previous suggestions of a low-mass (<5 M⊙) black hole.
Type
Refereed
Black hole physics

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