RA Dec
|
ℓ b
|
| Location in Globular Cluster | NGC 1851 | |
|---|---|---|
| Type of accretor | NS | Persistent |
|
Distance [kpc] (other distances) |
11.951
+0.134-0.133 |
Baumgardt2021 Harris2010Kuulkers2003Watkins2015Galloway2020 |
| z [kpc] | -6.89 | Baumgardt2021 |
| Orbital period (Porb) [min] | 17 | Zurek2009 |
| Porb determination method | UV modulation | |
| Thermonuclear X-ray burst | Short-B | Forman1976bGalloway2020 |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
1.33E-10 | Fiocchi2011 |
| NH [x1022 cm-2] | 0.026 | Sidoli2001 |
| E(B-V) [mag] | 0.02±0.01 | Harris2010 |
| Magnitude | B=21.1 | Deutsch1996 |
| Proposed companion |
| The orbital period is confirmed by detections in soft X-rays (Fiocchi2011). Fiocchi2011 suggested a high inclination angle of the binary system (> 80 deg). 4U 0513-40 shows large X-ray flux variations of more than a factor of 10 on time-scales of days to weeks (Maccarone2010). |
| UV | ||
|---|---|---|
| Optical | ||
| X-ray | Interstellar O absorption line (23.4 Å) | Juett2005 |
|
|||
|---|---|---|---|
| U=20.2, B=21.1 | |||