RA Dec
|
ℓ b
|
Location in Globular Cluster | ||
---|---|---|
Type of accretor | NS | Persistent |
Distance [kpc] (other distances) |
6.2(H), 9.5(He)
|
Degenaar2010b |
z [kpc] | -0.29 | Degenaar2010b |
Orbital period (Porb) [min] | ||
Porb determination method | ||
Thermonuclear X-ray burst | IB |
Degenaar2010b |
Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
2.30E-12 | ArmasPadilla2013b |
NH [x1022 cm-2] | 1.4±0.1 | ArmasPadilla2013b |
E(B-V) [mag] | ||
Magnitude | V=21.2 | Degenaar2010b |
Proposed companion |
In the optical spectra narrow Hα and Ca II emission lines are present, which are suggested to arise from de accretion disk or in the hemisphere of the secondary facing the neutron star due to X-ray resprocession (Degenaar2010b). |
UV | ||
---|---|---|
Optical | Hα Ca II λ8498 and λ8542, O I λ8446 emission lines | Degenaar2010b |
X-ray | Featureless | ArmasPadilla2013b |
|
|||
---|---|---|---|
V=21.2, R =18.8, J=15.4, H=14.3, K=13.8, R>17.5, B>23 |