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. New outburst reported on June 2025 (Sun2025). |
|
|||
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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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