RA Dec
|
ℓ b
|
| Location in Globular Cluster | ||
|---|---|---|
| Type of accretor |
NS AMXP (435.32 Hz / 2.30 ms) |
Transient Markwardt2002 |
|
Distance [kpc] (other distances) |
assumed 8.5
|
Gierlinski2005 Markwardt2002Papitto2008 |
| z [kpc] | -0.28 | Gierlinski2005 |
| Orbital period (Porb) [min] | 42.42235±0.00006 | Markwardt2002 |
| Porb determination method | X-ray pulsation | |
| Thermonuclear X-ray burst | ||
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
1.27E-09 | Gierlinski2005 |
| NH [x1022 cm-2] | 1.000+0.023-0.011 | Gierlinski2005 |
| E(B-V) [mag] | ||
| Magnitude | R>23.1 | Jonker2003b |
| Proposed companion | (warm helium dwarf) ( companion mass vs radius plane) |
-- Markwardt2002 |
| The source was not detected in quiescence with a 3σ upper limit on the count rate of 1.2E-4 counts/s (0.5-7 keV; Wijnands2005). Combining the timing solution for the 2002 and 2009 outbursts Riggio2011 found the orbital period derivative to be in the interval from -2.7E-11 to 0.7E-11 s/s (1σ). |
| UV | ||
|---|---|---|
| Optical | ||
| X-ray | Featureless | Miller2003 |
|
|||
|---|---|---|---|
| R>23.1, I>21.6, Z>20.6, J>19.6, K>19.2 | |||
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