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 |
|
|||
---|---|---|---|
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 |