RA Dec
|
ℓ b
|
| Location in Globular Cluster | ||
|---|---|---|
| Type of accretor | NS | Persistent |
|
Distance [kpc] (other distances) Gaia [kpc] |
3.0±0.1 (H), 3.8±0.2 (He)
2.03+1.17-2.3 2.0+1.2-2.4 |
Galloway2020 IntZand2008 BailerJones2018 Arnason2021 |
| z [kpc] | 0.25 | Galloway2020 |
| Orbital period (Porb) [min] | ||
| Porb determination method | ||
| Thermonuclear X-ray burst | Short-B IB |
Boller1997Piro1997 IntZand2008 |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
9.10E-11 | IntZand2008 |
| NH [x1022 cm-2] | 0.5 | IntZand2008 |
| E(B-V) [mag] | ||
| Magnitude | V=19.45 | Bassa2006 |
| Proposed companion |
| 1258-Hz high amplitude kilohertz QPO (Jonker2007a). Radio flux density < 21 μJy (5GHz), < 24 μJy (9GHz; VanDenEijnden2021). |
| UV | ||
|---|---|---|
| Optical | Featureless | IntZand2008 |
| X-ray | O (~0.54 keV) and Ne (~0.87 keV) absorption K-edges, Fe (~0.7 keV) absorption L-edge | IntZand2008 |
|
|||
|---|---|---|---|
| V=19.45 | |||