RA Dec
|
ℓ b
|
| Location in Globular Cluster | ||
|---|---|---|
| Type of accretor | NS | Transient (Long outburst) |
|
Distance [kpc] (other distances) |
<5.3 (H), <8.4 (He)
|
degenaar2011_burstxmmsource |
| z [kpc] | 0.01 | degenaar2011_burstxmmsource |
| Orbital period (Porb) [min] | ||
| Porb determination method | ||
| Thermonuclear X-ray burst | Short-B IB |
Brandt2006 degenaar2011_burstxmmsource |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
6.40E-12 | degenaar2011_burstxmmsource |
| NH [x1022 cm-2] | 8.9±0.5 | DelSanto2007 |
| E(B-V) [mag] | ||
| Magnitude | H=15.3±0.1 | Degenaar2007 |
| Proposed companion |
| Kaur2017 found two NIR counterpart candidates of the source. However, given that these candidates seem to be high-mass stars and that the color-color diagram indicates that they are part of the field population, the authors suggest that these are actually field stars. An analogous analysis was presented by Zolotukhin2015. |
| UV | ||
|---|---|---|
| Optical | ||
| X-ray |
|
|||
|---|---|---|---|
| H=15.3±0.1 | |||
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