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

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ID# 27

XTE J1550-564

V381 Nor

(Corbel2001)

RA     (ICRS)     DEC

[hh:mm:ss.ss]          [dd:mm:ss.ss]

15:50:58.70  -56:28:35.20


ℓ                      b

[deg]                            [deg]

325.8824005  -01.82687035

Year of discovery: 1998  
(Smith1998a)

# of outbursts after discovery: 5


Basic data

Distance [kpc] 4.5±0.5 Orosz2011aOrosz2002
Distance to the plane (z) [kpc] -0.14±0.02 Orosz2011aOrosz2002
Orbital period (Porb) [h] 37.0088±0.0001 Orosz2011aOrosz2002
Peak X-ray flux [erg s-1 cm-2]
[keV]
1.61E-07
[2-10]
Wu2002
Outburst magnitude (AB) V∼16.6 Orosz2002
Quiescent magnitude (AB) V=22.0±0.2 Orosz2002Orosz2011aCalvelo2010Jain2001
E(B-V) [mag] 1.33 Orosz2011a

Dynamically confirmed BH


NOTES

XTE J1550-564 showed a second complete outburst in 2000 (Smith2000a) and other three faint mini-outbursts in 2001, 2002 and 2003 (Tomsick2001,Belloni2002,Dubath2003).

Dynamical parameters

Orbital period [h] 37.0088±0.0001 Orosz2011aOrosz2002
Star's spectral type K2 – 4IV Orosz2011aOrosz2002
Star's radial velocity amplitude (K2) [km/s] 363±6 Orosz2011aOrosz2002
Mass function 'f(M1)' [M] 7.7±0.4 Orosz2011aOrosz2002
BH mass (M1) [M] 7.8 – 15.6 Orosz2011aOrosz2002
Mass ratio (q=M2/M1) ≈0.03 Orosz2011aOrosz2002
Inclination angle (i) [deg] 75±4 Orosz2011aOrosz2002
Rot. broadening (v sini) [km/s] 55±5 Orosz2011aOrosz2002



Optical/NIR magnitudes

Mag. Outburst (AB)
Orosz2002
V∼16.6
Mag. Quiescent (AB)
Orosz2002Orosz2011aCalvelo2010Jain2001
B>23.8±0.1 V=22.0±0.2 R∼22
i=19.04±0.03
J=19.24±0.04 H=17.6±0.1 Ks=18.00±0.04
Aladin finding chart
Scroll to zoom. Set survey image in "Manage layers"
Default image: DSS2 Red
XTE J1550-564 in Simbad

Finding charts

Orientation: North up, East left. Object marked
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Finding chart
Finding chart
Finding chart
Finding chart
Finding chart


Comparison stars (AB mag)

Jain2001a
B117.0±0.2 V116.2±0.2 R115.6±0.2
B217.6±0.2 V216.0±0.2 R214.7±0.1
B316.7±0.1 V315.8±0.2 R315.0±0.2
B916.3±0.2 V914.5±0.2 R911.9±0.2
B1015.7±0.1 V1014.4±0.2 R1013.3±0.1
B1117.4±0.2 V1116.5±0.2 R1115.8±0.2
B1214.5±0.1 V1213.4±0.2 R1212.5±0.1
B1317.0±0.1 V1315.8±0.2 R1314.7±0.1
B1417.2±0.2 V1415.9±0.2 R1414.8±0.2
B1515.4±0.1 V1513.5±0.2 R1511.4±0.2
B1617.2±0.2 V1616.1±0.2 R1615.0±0.4
B1716.9±0.2 V1715.4±0.2 R1714.0±0.2
B1817.5±0.2 V1816.0±0.2 R1814.6±0.2
B1916.3±0.1 V1914.9±0.2 R1913.7±0.1
B2016.9±0.2 V2015.5±0.2 R2014.5±0.1
B2117.0±0.2 V2115.2±0.2 R2113.6±0.2
B2216.0±0.1 V2214.8±0.2 R2213.9±0.1
B2316.1±0.1 V2315.2±0.2 R2314.6±0.1
B2417.4±0.2 V2416.6±0.2 R2415.8±0.2
B2515.1±0.1 V2514.5±0.2 R2514.0±0.1
B2617.1±0.2 V2615.8±0.2 R2614.7±0.2
B2714.4±0.1 V2714.0±0.2 R2714.0±0.1
B2815.4±0.1 V2813.8±0.2 R2812.3±0.2
J 115.6±0.3 H 115.7±0.3 Ks116.1±0.2
J 214.0±0.2 H 213.7±0.2 Ks214.0±0.2
J 314.9±0.3 H 314.9±0.2 Ks315.2±0.2
J 415.5±0.3 H 415.3±0.2 Ks415.6±0.2
J 514.9±0.3 H 514.7±0.2 Ks515.0±0.3
J 614.8±0.3 H 614.8±0.2 Ks615.2±0.3
J 715.3±0.3 H 715.0±0.2 Ks715.3±0.2
J 815.0±0.3 H 814.8±0.2 Ks815.1±0.2



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.