RA Dec
|
ℓ b
|
| Location in Globular Cluster | ||
|---|---|---|
| Type of accretor | NS | Persistent |
|
Distance [kpc] (other distances) Gaia [kpc] |
9.2±2.3 (He)
3.3-1.4+6.5 |
Serino2018 Wang2004 BailerJones2018 |
| z [kpc] | -1.02 | Serino2018 |
| Orbital period (Porb) [min] | 18.2±0.1 | Wang2004 |
| Porb determination method | Optical modulation | |
| Thermonuclear X-ray burst | Short-B | Serino2018 |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
7.27E-10 | Juett2003b |
| NH [x1022 cm-2] | 0.35 | Juett2003b |
| E(B-V) [mag] | ||
| Magnitude | r' = 20.42±0.03 | Wang2004 |
| Proposed companion | CO WD;
ONe WD (Optical spectrum; X-ray spectral modelling) |
Nelemans2004 Juett2001 |
| Radio luminosity < 7.2E27 erg/s (5GHz; Tetarenko2018). Radio flux < 6 mJy (2 cm; Duldig1979). |
| UV | ||
|---|---|---|
| Optical | Shallow CO emission lines | Nelemans2004 |
| X-ray | Ne/O (0.7 keV) Fe Kα (6.4 keV) |
Juett2003b Farinelli2003Madej2011 |
|
|||
|---|---|---|---|
| B~20, r' = 20.42±0.03 | |||