RA (ICRS) DEC
|
ℓ b
|
Distance [kpc] | 1.06±0.1 | Cantrell2010 |
---|---|---|
Distance to the plane (z) [kpc] | -0.11±0.01 | Cantrell2010 |
Orbital period (Porb) [h] | 7.752340±2E-06 | GonzalezHernandez2014 |
Peak X-ray flux [erg s-1 cm-2] [keV] |
2.65E-06 [2-10] |
Warwick1981 |
Outburst magnitude (AB) | V∼11.1 | Robertson1976 |
Quiescent magnitude (AB) | V=18.23±0.04 | Cantrell2010Gelino2001Froning2001 |
E(B-V) [mag] | 0.35 | Hynes2005 |
Dynamically confirmed BH
3A 0620-003 showed an outburst in 1917 detected in plate scales prior to its detection in X-rays in 1975 (Eachus1976). A period derivative of -0.60±0.08 ms/yr has been measured (GonzalezHernandez2014). Gandhi2019 obtained a distance of 1.72+1.02-0.47 kpc from Gaia DR2. |
Orbital period [h] | 7.752340±2E-06 | GonzalezHernandez2014 |
---|---|---|
Star's spectral type | K2 – 7V | Orosz1994 |
Star's radial velocity amplitude (K2) [km/s] | 437±2 | GonzalezHernandez2010 |
Mass function 'f(M1)' [M☉] | 2.79±0.04 | GonzalezHernandez2010 |
BH mass (M1) [M☉] | 6.6±0.3 | Cantrell2010 |
Mass ratio (q=M2/M1) | 0.074±0.006 | Orosz1994 |
Inclination angle (i) [deg] | 51±0.9 | Cantrell2010 |
|
|||
---|---|---|---|
B∼11.3 | V∼11.1 | ||
Cantrell2010Gelino2001Froning2001 |
|||
B=19.32±0.04 | V=18.23±0.04 | R=17.12±0.04 | |
I=17.01±0.04 | |||
J=16.5±0.1 | H=16.23±0.02 |
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