RA Dec
|
ℓ b
|
Location in Globular Cluster | ||
---|---|---|
Type of accretor | NS | Transient (Long outburst) |
Distance [kpc] (other distances) |
<4.8 (H), <6.2 (He)
|
Galloway2020 Cornelisse2002a |
z [kpc] | -0.08 | Galloway2020 |
Orbital period (Porb) [min] | ||
Porb determination method | ||
Thermonuclear X-ray burst | Short-B
IB |
Cornelisse2002a IntZand2019 |
Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
6.60E-10 | delsanto2012 |
NH [x1022 cm-2] | 4.2±0.6 | delsanto2012 |
E(B-V) [mag] | ||
Magnitude | K=17.25±0.03 qK>18.2 |
Kaur2017 Kaur2017 |
Proposed companion |
The source was still detected by INTEGRAL in 2015 October (Sguera2015). |
UV | ||
---|---|---|
Optical | ||
X-ray | Featureless | Degenaar2011b |
|
|||
---|---|---|---|
K=17.25±0.03, qK>18.2, H=17.94±0.06, K_s = 17.22±0.02, qH>19.00 |
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