RA Dec
|
ℓ b
|
| Location in Globular Cluster | ||
|---|---|---|
| Type of accretor | NS | Persistent |
|
Distance [kpc] (other distances) |
2.3(H), 3(He)
|
Galloway2020 Jonker2004Chelovekov2011 |
| z [kpc] | 0.10 | Galloway2020 |
| Orbital period (Porb) [min] | 114 | ArmasPadilla2022 |
| Porb determination method | Optical modulation | |
| Thermonuclear X-ray burst | Short-B | Murakami1983Tarana2006 IntZand2019Galloway2020 |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
3.80E-10 | Muno2005b |
| NH [x1022 cm-2] | 1.50 | Tarana2006Barret2003 |
| E(B-V) [mag] | ||
| Magnitude | r=22.7 | ArmasPadilla2020 |
| Proposed companion | evolved main-sequence star with a low fraction of photospheric hydrogen as donor star (Optical spectra, Bursts) |
ArmasPadilla2022 |
| UV | ||
|---|---|---|
| Optical | Featureless | ArmasPadilla2022 |
| X-ray |
|
|||
|---|---|---|---|
| r=22.7, g=25.3, rs = 23.17 ± 0.02, is = 21.93 ± 0.01, zs = 21.28 ± 0.01, R= 22.15 | |||
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