2016MNRAS.463.1314S

Query : 2016MNRAS.463.1314S

2016MNRAS.463.1314S - Mon. Not. R. Astron. Soc., 463, 1314-1322 (2016/December-1)

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

SHAW A.W., CHARLES P.A., CASARES J. and HERNANDEZ SANTISTEBAN J.V.

Abstract (from CDS):

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.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): black hole physics - X-rays: binaries - X-rays: individual: Swift J1753.5-0127 - X-rays: individual: Swift J1753.5-0127

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 V* V518 Per HXB 04 21 42.7227473352 +32 54 26.939156184           M4.5V 670 0
2 V* KV UMa HXB 11 18 10.7930420496 +48 02 12.314730120           K5V-M1V 865 0
3 * 38 Com * 13 01 09.6152814960 +17 07 23.327673312   6.90 5.93     G9III 49 0
4 * 40 Com LP* 13 06 22.6020265896 +22 36 58.273099308 8.82 7.22 5.61 3.63 1.84 M5III: 115 0
5 HD 114326 PM* 13 09 47.8475594496 +16 50 55.004141976 9.01 7.32 5.87     K4III 57 0
6 HD 114780 PM* 13 12 32.9201305680 +11 33 21.958827804   7.28 5.77     M0III 39 0
7 BD+33 2642 pA* 15 51 59.8854348048 +32 56 54.329485272 9.806 10.61 10.73 10.884 10.961 O7p 456 0
8 2MAXI J1753-013 LXB 17 53 28.2898766424 -01 27 06.256555272 15.30 16.73 16.46 16.15 15.64 ~ 384 0

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