RA Dec
|
ℓ b
|
| Location in Globular Cluster | ||
|---|---|---|
| Type of accretor |
NS AMXP (185.11 Hz / 5.40 ms) |
Transient Remillard2002 |
|
Distance [kpc] (other distances) |
assumed 10
|
Campana2005 |
| z [kpc] | 2.46 | Campana2005 |
| Orbital period (Porb) [min] | 43.57910±0.00005 | Galloway2002 |
| Porb determination method | X-ray pulsation | |
| Thermonuclear X-ray burst | ||
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
2.70E-10 | Juett2003a |
| NH [x1022 cm-2] | 0.076 | Juett2003a |
| E(B-V) [mag] | ||
| Magnitude | V=18.63±0.03 qV=27.58±0.12 |
Giles2005 Monelli2005 |
| Proposed companion | C/O system (Opt spectra) |
Nelemans2006 |
| A radio counterpart was identified during the 2002 outburst (4.86GHz; Rupen2002b). The source was detected during quiescence with an unabsorbed flux of ~6E-15 erg s-1 cm-2 (0.5-10 keV; Campana2005, Wijnands2005). |
| UV | ||
|---|---|---|
| Optical | Emission at ~4640 Å (C or N) | Nelemans2006 |
| X-ray | Interstellar O absorption line (23.52 Å) | Juett2003a |
|
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|---|---|---|---|
|
I=18.14±0.04, B=18.45±0.01, V=18.63±0.03, R=18.83±0.02 qV=27.58±0.12, qR=27.21±0.13, qI=27.23±0.22 |
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