RA (ICRS) DEC
|
ℓ b
|
Distance [kpc] |
3.46+2.18-1.03/ 2.96±0.33 |
Gandhi2019Atri2020 |
---|---|---|
Distance to the plane (z) [kpc] | 0.61±0.380.18 / 0.52 | Gandhi2019Atri2020 |
Orbital period (Porb) [h] | 16.4518±0.0002 | Torres2019 |
Peak X-ray flux [erg s-1 cm-2] [keV] |
2.26E-07 [2-10] |
Tucker2018 |
Outburst magnitude (AB) | V∼14 | Tucker2018 |
Quiescent magnitude (AB) | V=18.3 | Hambsch2019 |
E(B-V) [mag] | 0.18 | Tucker2018 |
Dynamically confirmed BH
MAXI J1820+070: Kojiguchi2019 identified historic outburst in 1898 and 1934 through the analysis of photographic plates (suggesting a recurrence of 40 yr) and it showed rebrightenings in Jan 2019 (Russell2019c), Aug 2019 (Hambsch2019), Feb 2020 (Adachi2020) and Mar 2021 (Baglio2021) |
Orbital period [h] | 16.4518±0.0002 | Torres2019 |
---|---|---|
Star's spectral type | K3 – 5 | Torres2019 |
Star's radial velocity amplitude (K2) [km/s] | 418±4 | Torres2019 |
Mass function 'f(M1)' [M☉] | 5.2±0.2 | Torres2019 |
BH mass (M1) [M☉] | 5.71 – 8.10 (8.40±0.770.70 if adopted i=63º) | Torres2020 |
Mass ratio (q=M2/M1) | 0.07±0.01 | Torres2020 |
Inclination angle (i) [deg] | >67 – 81 (or 63±3 for the orientation angle of the radio jet) | Torres2020Atri2020 |
Rot. broadening (v sini) [km/s] | 84±5 | Torres2020 |
|
|||
---|---|---|---|
V∼14 | g’=13.14±0.03 | i’=13.08±0.05 | |
Hambsch2019 |
|||
V=18.3 | |||
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