RA (ICRS) DEC
|
ℓ b
|
Distance [kpc] | 9.4±0.8 | Reid2023 |
---|---|---|
Distance to the plane (z) [kpc] | -0.034±0.01 | Reid2023 |
Orbital period (Porb) [h] | 812±4 | Steeghs2013 |
Peak X-ray flux [erg s-1 cm-2] [keV] |
9.29E-08 [2-10] |
XTE/ASM |
Outburst magnitude (AB) | H=13.09 | Shahbaz2008 |
Quiescent magnitude (AB) | I∼23.7±0.4 | Boeer1996 |
E(B-V) [mag] | 6.45 | Fender1999 |
Dynamically confirmed BH
GRS J1915+105 has remained in outburst since its discovery in 1992 (Castro-Tirado1992). It is included here because it was detected as a transient source. The peak X-ray flux was obtained from the maximum value in the XTE/ASM light curves (MJD=50317.68034). The K-band magnitude was not transformed into AB system. |
Orbital period [h] | 812±4 | Steeghs2013 |
---|---|---|
Star's spectral type | K1 – 5III | Harlaftis2004 |
Star's radial velocity amplitude (K2) [km/s] | 126±1 | Steeghs2013 |
Mass function 'f(M1)' [M☉] | 7±0.2 | Steeghs2013 |
BH mass (M1) [M☉] |
12 11.2±2 |
Reid2023 Steeghs2013Reid2014 |
Mass ratio (q=M2/M1) | 0.042±0.024 | Steeghs2013 |
Inclination angle (i) [deg] | 60±5 | Reid2023 |
Rot. broadening (v sini) [km/s] | 21±4 | Steeghs2013 |
|
|||
---|---|---|---|
H=13.09 | K (not AB)=11.4 | ||
Boeer1996 |
|||
I∼23.7±0.4 | |||
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