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) |
|
|||
|---|---|---|---|
| Ks=18.28±0.05 | |||
|
|||
| Ks=20.1±0.3 | |||
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Orientation: North up, East left.
Object marked
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Finding chart reference: Torres2007aLopez2019