RA (ICRS) DEC
|
ℓ b
|
Distance [kpc] | 7.25±1.25 | Greiner1996 |
---|---|---|
Distance to the plane (z) [kpc] | 0.15±0.03 | Greiner1996 |
Orbital period (Porb) [h] | ||
Peak X-ray flux [erg s-1 cm-2] [keV] |
7.20E-09 [2-10] |
MAXI |
Outburst magnitude (AB) | J=17.2±0.1 | Marti1997 |
Quiescent magnitude (AB) | J>20.1 | Chaty2002a |
E(B-V) [mag] | 2 – 4 | Marti1997 |
Spectral type | >F5V | Chaty2002a |
GRS 1739-278 showed another outburst in 2014 (Miller2015b,Krimm2014b) and 2016 (Mereminskiy2016). The peak X-ray flux is taken from the MAXI SSC light curve of that outburst. It has an uncertain distance. Another outburst was reported on June 2023 by Negoro2023,Kennea2023 |
|
|||
---|---|---|---|
V=23.2±0.3 | R=20.6±0.1 | ||
J=17.2±0.1 | |||
Chaty2002a |
|||
J>20.1 | K (not AB)>18.4 |
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