RA (ICRS) DEC
|
ℓ b
|
Distance [kpc] | ||
---|---|---|
Distance to the plane (z) [kpc] | ||
Orbital period (Porb) [h] | ||
Peak X-ray flux [erg s-1 cm-2] [keV] |
7.46E-10 [2-10] |
Sala2008 |
Outburst magnitude (AB) | Ks=18.28±0.05 | Torres2007a |
Quiescent magnitude (AB) | Ks=20.1±0.3 | |
E(B-V) [mag] | 5.113 | Schlafly2011 |
Spectral type |
XTE J1856+053 has shown two consecutive outbursts with ∼70 days interval between them (Sala2008). This behaviour was seen in the 1996 and 2007 outbursts (Levine2007,Krimm2007,Sala2008). This also appeared in the the recent 2015 outburst (Suzuki2015,Negoro2015). A new outburst occurred in Feb 2020 (Negoro2020) |
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Ks=18.28±0.05 | |||
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Ks=20.1±0.3 |
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Orientation: North up, East left.
Object marked
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Finding chart reference: Torres2007aLopez2019