RA Dec
|
ℓ b
|
| Location in Globular Cluster | ||
|---|---|---|
| Type of accretor | NS | Persistent |
|
Distance [kpc] (other distances) |
<7.2±1.4 (H or He?)
|
Chelovekov2017 Lin2018Pavlinsky1994 |
| z [kpc] | -0.11 | Chelovekov2017 |
| Orbital period (Porb) [min] | ||
| Porb determination method | ||
| Thermonuclear X-ray burst | IB |
Pavlinsky1994IntZand2007Alizai2020 |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
2.08E-10 | Mori2005 |
| NH [x1022 cm-2] | 3.5 | Mori2005 |
| E(B-V) [mag] | ||
| Magnitude | I=23.37±0.28 | Zolotukhin2011 |
| Proposed companion |
| SLX 1744-299, first identified with a non-imaging instrument on board Spacelab-2, was later resolved into two sources separated by ~3’. The northern and southern components were then renamed as SLX 1744-299 and SLX 1744-300, respectively. |
| UV | ||
|---|---|---|
| Optical | ||
| X-ray | Featureless | Mori2005 |
|
|||
|---|---|---|---|
| I=23.37±0.28, J > 19.9, H > 18.7, K > 18 (Vega) | |||
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