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

ID# 50

SWIFT J1357.2-0933

RA (h:m:s)  DEC (º:':")  J2000:
13:57:16.82 -09:32:38.55
( Rau2011 )

Galactic l (º)  b (º)  J2000:
328.7018426  +50.0043094

Year of discovery: 2011  
( Krimm2011a )

# of outbursts after discovery:

Non-dynamical but there is either a mass function or a mass determination suggesting the presence of a BH


Basic data

Distance (d) >2.29 (kpc) MataSanchez2015
d above plane (z) >1.75 (kpc) MataSanchez2015
Orbital period 2.8±0.3 (h) Corral-Santana2013
Peak X-ray flux 2.23E-10
[2-10]
(erg/s/cm2) [keV] ArmasPadilla2013
Outburst magnitude (AB) r'=16.3±0.05 (mag) Rau2011
Quiescent magnitude (AB) r'=21.71±0.08 (mag) Shahbaz2013 ArmasPadilla2014a MataSanchez2015 Shahbaz2013
E(B-V) 0.037 (mag) Schlafly2011
Notes Swift J1357.2-0933 in rigour is not a dynamical BHT because it lacks a detection of the secondary star but it has a robust mass function determination ( Corral-Santana2013 , MataSanchez2015 ). The distance is still uncertain (see Rau2011 , Shahbaz2013 , MataSanchez2015 ).

Dynamical parameters

Orbital period 2.8±0.3 (h) Corral-Santana2013
Star's spectral type M2-4V MataSanchez2015
Star's radial velocity amplitude (K2) 967±49 (km/s) MataSanchez2015
Mass function 'f(M1)' 11±2.1 (M) MataSanchez2015
BH mass (M1) >8.3 (M) MataSanchez2015
Mass ratio (q=M/M1) ∼0.04 MataSanchez2015
Inclination angle (i) ∼90 (deg) Corral-Santana2013 MataSanchez2015
Rot. broadening (v sini) (km/s)

Optical/NIR magnitudes

Mag. Outburst (AB) Rau2011
r'
=16.3±0.05
Mag. Quiescence (AB) Shahbaz2013 ArmasPadilla2014a MataSanchez2015 Shahbaz2013
r' i' u' g' J
=21.71±0.08 =21.2±0.4 =23.12±0.04 =22.3±0.4 =20.51±0.06
H Ks g' r'
=20.07±0.05 =20.09±0.05 =22.29±0.08 =21.5±0.4
Scroll to zoom. Set survey image in Controls
Default image: DSS2 Red
SWIFT J1357.2-0933 in Simbad
Finding charts orientation:North up, East left
Click to enlarge in new tab/window
Object marked with lines


Comparison stars reference: Corral-Santana2013

Finding chart
Finding chart
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.