BlackCAT A Catalog of Stellar-Mass Black Holes in X-ray Binaries

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ID# 39

Swift J1753.5-0127

( Fender2005 )

RA     [J2000]     DEC

[hh:mm:ss.ss]          [dd:mm:ss.ss]

17:53:28.29  -01:27:06.22


ℓ                      b

[deg]                            [deg]

024.8976155  +12.18607327

Year of discovery: 2005  
( Palmer2005 )

# of outbursts after discovery:


Basic data

Distance [kpc] ∼6±2 CadolleBel2007
Distance to the plane (z) [kpc] ∼1.3±0.4 CadolleBel2007
Orbital period (Porb) [h] 3.244±0.001 Zurita2008
Peak X-ray flux [erg s-1 cm-2]
[keV]
5.64E-09
[2-10]
Soleri2013
Outburst magnitude (AB) R∼15.85 Halpern2005
Quiescent magnitude (AB) V>21.0 CadolleBel2007
E(B-V) [mag] 0.45 Rahoui2015

Strictly speaking it is not a dynamical BH but there is either a robust mass function or mass determination suggesting the presence of a BH


NOTES

Swift J1753.5-0127 remained in a low/hard X-ray state since its outburst in 2005 until 2016. In June 2015, it reached its lowest flux since its outburst ( Neustroev2015 ). After 11 years in outburst, it started to decay towards its quiescent state around September 2016 ( Russell2016 ). By early November 2016, the source was not detected in X-rays by Swift ( Shaw2016a ).
There is a discrepance between the K2,Porb and M1 measured by Neustroev2014 and Shaw2016 .
The FWHM(Hα) scaling ( Casares2015 ) coupled with the Porb ( Zurita2008 ) strongly indicates a BH ( Shaw2016 ).
Gandhi2019 obtained a distance of 7.15+3.99-2.48 kpc from Gaia DR2.

Dynamical parameters

Orbital period [h] 3.244±0.001 Zurita2008
Star's spectral type >M2 Zurita2008
Star's radial velocity amplitude (K2) [km/s] >808±76 Shaw2016
Mass function 'f(M1)' [M] 0.69±0.04 Neustroev2014
BH mass (M1) [M] >7.4±1.2 Shaw2016
Mass ratio (q=M2/M1) ≥0.04±0.03 Neustroev2014
Inclination angle (i) [deg] ≥40 Neustroev2014
Rot. broadening (v sini) [km/s]



Optical/NIR magnitudes

Mag. Outburst (AB)
Halpern2005
R∼15.85
Mag. Quiescent (AB)
CadolleBel2007
V>21.0
Aladin finding chart
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Swift J1753.5-0127 in Simbad

Pan-STARRS1 finding chart

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PS1 Finding chart PS1 Finding chart


This research has made use of NASA's Astrophysics Data System (ADS) and the SIMBAD database operated at CDS (Strasbourg, France)
Please acknowledge the use of this catalogue in any published work you derive from it.

Last modified: 27 August 2021.