RA Dec
|
ℓ b
|
| Location in Globular Cluster | ||
|---|---|---|
| Type of accretor | NS | Persistent |
|
Distance [kpc] (other distances) |
4.5±0.7(H), 5.8±0.9(He)
|
Galloway2020 Galloway2008Chelovekov2011Chelovekov2017Molkov2005 |
| z [kpc] | 0.24 | Galloway2020 |
| Orbital period (Porb) [min] | ||
| Porb determination method | ||
| Thermonuclear X-ray burst | Short-B
IB SB |
Bazzano1997 Molkov2005 Suzuki2005 |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
3.45E-10 | Wilson2003 |
| NH [x1022 cm-2] | 1.70±0.05 | Wilson2003 |
| E(B-V) [mag] | ||
| Magnitude | R=21.31±0.12 | Zolotukhin2011 |
| Proposed companion |
| Although the source is persistent, it showed an episode of enhanced activity in 2005 (IntZand2007). |
| UV | ||
|---|---|---|
| Optical | ||
| X-ray |
|
|||
|---|---|---|---|
| R=21.31±0.12, I=20.10±0.07, J > 19.4 | |||
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