RA Dec
|
ℓ b
|
| Location in Globular Cluster | NGC 6624 | |
|---|---|---|
| Type of accretor | NS | Persistent |
|
Distance [kpc] (other distances) |
8.019
+0.108-0.108 |
Baumgardt2021 Heasley2000Kuulkers2003Harris2010Galloway2020 |
| z [kpc] | -1.10 | Baumgardt2021 |
| Orbital period (Porb) [min] | 11.42 | Stella1987 |
| Porb determination method | X-ray modulation | |
| Thermonuclear X-ray burst | Short-B SB |
Clark1977 Strohmayer2002a |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
5.02E-09 | Costantini2012 |
| NH [x1022 cm-2] | 0.16±0.003 | Sidoli2001 |
| E(B-V) [mag] | 0.28 ± 0.03 | Harris2010 |
| Magnitude | B=18.7 | King1993a |
| Proposed companion | He WD (Burst modelling) |
Cumming2003 |
| Wang2010 detected an UV modulation at 693.5±1.3 s, ~1% longer than the orbital period, interpreted as a superhump period. Moreover, the source shows a long term modulation at ~171 d in X-rays (e.g., Priedhorsky1984, Zdziarski2007,Chou2001b) Chou2001b measured an orbital period derivative of (-7.54±3.21)E-13 s/s. The source is detected in radio (Russell2021) |
| UV | ||
|---|---|---|
| Optical | ||
| X-ray | O VII, O VIII and Ne IX absorption lines (hot interstellar medium?) | Futamoto2004Cackett2008 |
|
|||
|---|---|---|---|
| B=18.7 | |||
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