RA (ICRS) DEC
|
ℓ b
|
Distance [kpc] | 2.39±0.14 | Miller-Jones2009 |
---|---|---|
Distance to the plane (z) [kpc] | -0.09±0.01 | Miller-Jones2009 |
Orbital period (Porb) [h] | 155.30803±5E-05 | Casares2019 |
Peak X-ray flux [erg s-1 cm-2] [keV] |
2.59E-07 [2-10] |
Zycki1999 |
Outburst magnitude (AB) | R∼10.7 | Casares1991 |
Quiescent magnitude (AB) | R=16.58±0.01 | Casares1993Zurita2004 |
E(B-V) [mag] | 1.3 | Casares1993 |
Dynamically confirmed BH
GS 2023+338 (V404 Cyg) showed two outbursts detected in plate scales (1938 and 1956) prior to its detection in X-rays in 1989 (Wachmann1948,Richter1989). It has shown two new outbursts in 2015: June (Barthelmy2015) and December (Barthelmy2015a). Gandhi2019 obtained a distance of 2.40+0.95-0.53 from Gaia DR2. |
Orbital period [h] | 155.30803±5E-05 | Casares2019 |
---|---|---|
Star's spectral type | K3III | Casares1993Khargharia2010 |
Star's radial velocity amplitude (K2) [km/s] | 208.4±0.5 | Casares2019 |
Mass function 'f(M1)' [M☉] | 6.08±0.06 | Casares1992Casares1994 |
BH mass (M1) [M☉] | 9+0.2-0.6 | Khargharia2010 |
Mass ratio (q=M2/M1) | 0.067±0.005 | Casares1994Casares1996 |
Inclination angle (i) [deg] | 67+3-1 | Khargharia2010 |
Rot. broadening (v sini) [km/s] | 39±1 | Casares1996 |
|
|||
---|---|---|---|
V∼11.7 | R∼10.7 | ||
Casares1993Zurita2004 |
|||
B=20.47±0.05 | V=18.38±0.02 | R=16.58±0.01 | |
I=16.07±0.05 | |||
J=14.59±0.08 | H=14.21±0.06 | Ks=14.39±0.05 |
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