RA (ICRS) DEC
|
ℓ b
|
Distance [kpc] | 7.5+1.8-1.4 | MataSanchez2021 |
---|---|---|
Distance to the plane (z) [kpc] | -1.0±0.2 | MataSanchez2021 |
Orbital period (Porb) [h] |
9.5±0.1 9.74±0.04 |
MataSanchez2021Shidatsu2013 |
Peak X-ray flux [erg s-1 cm-2] [keV] |
1.03E-09 [2-10] |
Morihana2013 |
Outburst magnitude (AB) | i’=16.61±0.05 | Greiner2012 |
Quiescent magnitude (AB) | i’=20.21±0.08 | MataSanchez2021 |
E(B-V) [mag] | 0.18 | MataSanchez2021 |
Dynamically confirmed BH
MAXI J1305-704 showed X-ray dips during the outburst (Shidatsu2013). There is a contaminant star 1.64” North of the object (MataSanchez2021). The values of M1 and M2 are the most conservative given the different results of the inclination obtained from the photometric modelling. The best fit of the inclination (i=72+5-8 deg) would imply 9.0+1.5-1.0 and 0.43±0.16 M☉ for M1 and M2 respectively (MataSanchez2021). |
Orbital period [h] |
9.5±0.1 9.74±0.04 |
MataSanchez2021Shidatsu2013 |
---|---|---|
Star's spectral type | K3 – 5 | MataSanchez2021 |
Star's radial velocity amplitude (K2) [km/s] | 554±8 | MataSanchez2021 |
Mass function 'f(M1)' [M☉] | 6.9±0.3 | MataSanchez2021 |
BH mass (M1) [M☉] | 8.9+1.6-1.0 | MataSanchez2021 |
Mass ratio (q=M2/M1) | 0.05±0.02 | MataSanchez2021 |
Inclination angle (i) [deg] | 60 – 82 | MataSanchez2021 |
Rot. broadening (v sini) [km/s] | <110 (84% c.l.) | MataSanchez2021 |
|
|||
---|---|---|---|
uvw1=17.23±0.04 | g’=16.51±0.05 | r’=16.50±0.05 | i’=16.61±0.05 |
z’=16.65±0.05 | J=16.52±0.05 | H=16.59±0.05 | |
MataSanchez2021 |
|||
g’=21.78±0.10 | |||
r’=20.60±0.07 | i’=20.21±0.08 | z’=19.93±0.06 | |
Orientation: North up, East left.
Object marked
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Finding chart reference: MataSanchez2021