RA (ICRS) DEC
|
ℓ b
|
| Distance [kpc] | 6.2±0.7 | MacDonald2014 |
|---|---|---|
| Distance to the plane (z) [kpc] | -0.52±0.06 | MacDonald2014 |
| Orbital period (Porb) [h] | 67.6152±0.0002 | Orosz2001 |
| Peak X-ray flux [erg s-1 cm-2] [keV] |
2.76E-07 [2-10] |
Orosz2001 |
| Outburst magnitude (AB) | V=8.8 | Orosz2001 |
| Quiescent magnitude (AB) | V=13.96±0.02 | MacDonald2014Orosz2001 |
| E(B-V) [mag] | 0.32 – 0.38 | MacDonald2014 |
Dynamically confirmed BH
| SAX J1819.3-2525 (V4641 Sgr) showed weak outbursts in 2002 ,2003 (Bailyn2003), 2010 (Yamaoka2010), 2014 (Tachibana2014) and 2018 (Negoro2018), and a complete outburst in 2015 (Yoshii2015) and 2020 (Shaw2020). A new outburst was reported on Sep 2024 (Negoro2024) Gandhi2019 obtained a distance of 6.24+2.04-1.30 kpc from Gaia DR2. |
| Orbital period [h] | 67.6152±0.0002 | Orosz2001 |
|---|---|---|
| Star's spectral type | B9III | Orosz2001 |
| Star's radial velocity amplitude (K2) [km/s] | 211±3 | Orosz2001 |
| Mass function 'f(M1)' [M☉] | 2.7±0.1 | Orosz2001 |
| BH mass (M1) [M☉] | 6.4±0.6 | MacDonald2014 |
| Mass ratio (q=M2/M1) | 0.63 – 0.70 | MacDonald2014 |
| Inclination angle (i) [deg] | 72±4 | MacDonald2014 |
| Rot. broadening (v sini) [km/s] | 100.9±0.8 | MacDonald2014 |
|
|||
|---|---|---|---|
| V=8.8 | |||
MacDonald2014Orosz2001 |
|||
| B∼13.91±0.04 | V=13.96±0.02 | R=13.73±0.02 | |
| I=13.52±0.03 | |||
| J=14.86±0.05 | H=14.23±0.05 | K=12.83±0.05 | |
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Object marked
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