RA Dec
|
ℓ b
|
Location in Globular Cluster | ||
---|---|---|
Type of accretor | NS | Persistent |
Distance [kpc] (other distances) Gaia [kpc] |
3.0±0.2 (H), 3.9±0.2 (He)
4.0 5.77+2.77-1.60 |
Galloway2020 Jonker2004IntZand2005b VanDenEijnden2021 BailerJones2018 |
z [kpc] | -0.26 | Galloway2020 |
Orbital period (Porb) [min] | 17.4±0.1 | Zhong2011 |
Porb determination method | Optical modulation | |
Thermonuclear X-ray burst | Short-B IB |
Jonker2001b IntZand2005 |
Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
1.12E-10 | Juett2003b |
NH [x1022 cm-2] | 0.3 | Juett2003b |
E(B-V) [mag] | ||
Magnitude | V = 20.98±0.07 | Chevalier1987 |
Proposed companion | He WD;
CO WD;
ONe WD (Burst modelling; optical spectrum; X-ray spectral modelling) |
IntZand2005b Nelemans2004Nelemans2006 Juett2001 |
Radio flux density < 20 μJy (5.5 GHz; VanDenEijnden2021. According to the authors, the source was not detected at radio frequencies; the radio luminosity < ~3E27 erg/s). Fradio < 6 mJy (2 cm (14.7GHz); Duldig1979). |
UV | ||
---|---|---|
Optical | Featureless (see, however, Nelemans2004 and Nelemans2006 for a marginal CO detection). | Nelemans2004Nelemans2006 |
X-ray | Ne (0.7 keV) | Juett2001 |
|
|||
---|---|---|---|
V = 20.98±0.07, B = 21.29±0.07, r' = 20.95±0.16 |