RA (ICRS) DEC
|
ℓ b
|
| Distance [kpc] | 7.5±0.5 | Jonker2004 |
|---|---|---|
| Distance to the plane (z) [kpc] | 0.7±0.05 | Jonker2004 |
| Orbital period (Porb) [h] | 26.79377±0.00007 | Orosz1998Orosz2003 |
| Peak X-ray flux [erg s-1 cm-2] [keV] |
9.42E-08 [2-10] |
Park2004 |
| Outburst magnitude (AB) | V=13.90 | Saikia2021a |
| Quiescent magnitude (AB) | V=16.7 | Orosz1998Chevalier1992Buxton2004 |
| E(B-V) [mag] | 0.5 | Orosz1998 |
Dynamically confirmed BH
| 4U 1543-475 have shown outbursts in 1984, 1992, 2002 and 2021 (Kitamoto1984,Harmon1992a,Miller2002,Negoro2021). The peak X-ray flux is taken from the 2002 outburst (Park2004). Gandhi2019 obtained a distance of 8.60+3.84-2.46 kpc from Gaia DR2. The 2021 outburst was brighter than the previous ones, perhaps super-Eddington, with Saikia2021a reporting outburst magnitudes ~1 mag brighter than previous outbursts when the system was still brightening. |
| Orbital period [h] | 26.79377±0.00007 | Orosz1998Orosz2003 |
|---|---|---|
| Star's spectral type | A2V | Orosz1998 |
| Star's radial velocity amplitude (K2) [km/s] | 124±4 | Orosz1998 |
| Mass function 'f(M1)' [M☉] | 0.25±0.01 | Orosz1998Orosz2003 |
| BH mass (M1) [M☉] | 8.4 – 10.4 | Orosz1998Orosz2003 |
| Mass ratio (q=M2/M1) | 0.25 – 0.31 | Orosz1998Orosz2003 |
| Inclination angle (i) [deg] | 20.7±1.5 | Orosz1998Orosz2003 |
| Rot. broadening (v sini) [km/s] | 46±2 | Orosz1998Orosz2003 |
|
|||
|---|---|---|---|
| B=14.53 | V=13.90 | R=13.54 | i’=13.60 |
Orosz1998Chevalier1992Buxton2004 |
|||
| B=17.3 | V=16.7 | ||
| I=16.1±0.1 | |||
| J=16.04±0.05 | |||
| Light Curve by XB-NEWS (Russell2019) |