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

« Previous BHT   Next BHT »

ID# 16

GRS 1124-684

N Mus 1991 = GU Mus

(dellaValle1991a)

RA     (ICRS)     DEC

[hh:mm:ss.ss]          [dd:mm:ss.ss]

11:26:26.65  -68:40:32.83


ℓ                      b

[deg]                            [deg]

295.3006588  -07.07263349

Year of discovery: 1991  
(Lund1991Makino1991)

# of outbursts after discovery:


Basic data

Distance [kpc] 4.95+0.69-0.65 Wu2016
Distance to the plane (z) [kpc] -0.73±0.04 Wu2016
Orbital period (Porb) [h] 10.38252±2E-05 GonzalezHernandez2017
Peak X-ray flux [erg s-1 cm-2]
[keV]
1.36E-07
[2-10]
Brandt1992
Outburst magnitude (AB) V∼13.5 dellaValle1991a
Quiescent magnitude (AB) i'=19.92±0.04 King1996aShahbaz1997Shahbaz2010
E(B-V) [mag] 0.3 dellaValle1991a

Dynamically confirmed BH


NOTES

GRS 1124-684 (N Mus91): A period derivative has been measured (GonzalezHernandesz2017).
Gandhi2019 obtained a distance of 2.71+3.82-1.38 kpc from Gaia DR2.

Dynamical parameters

Orbital period [h] 10.38252±2E-05 GonzalezHernandez2017
Star's spectral type K3 – 5V Orosz1996Casares1997
Star's radial velocity amplitude (K2) [km/s] 407±3 Orosz1996Wu2015
Mass function 'f(M1)' [M] 3.02±0.06 Orosz1996Wu2015
BH mass (M1) [M] 11.0+2.1-1.4 Wu2016
Mass ratio (q=M2/M1) 0.079±0.007 Wu2015
Inclination angle (i) [deg] 43.2+2.1-2.7 Wu2016
Rot. broadening (v sini) [km/s] 85±3 Wu2015



Optical/NIR magnitudes

Mag. Outburst (AB)
dellaValle1991a
V∼13.5
Mag. Quiescent (AB)
King1996aShahbaz1997Shahbaz2010
u'=21.5±0.4 g'=20.65±0.05
i'=19.92±0.04
J=19.05±0.02 H∼18.39 K (not AB)=17.08±0.01
Aladin finding chart
Scroll to zoom. Set survey image in "Manage layers"
Default image: DSS2 Red
GRS 1124-684 in Simbad

Finding charts

Orientation: North up, East left. Object marked
Click to enlarge in new tab/window

Finding chart


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

Last modified: 25 March 2024.