RA Dec
|
ℓ b
|
Location in Globular Cluster | ||
---|---|---|
Type of accretor | NS | Transient |
Distance [kpc] (other distances) |
<5.8 (He)
|
Chenevez2012 Chelovekov2017 |
z [kpc] | -0.62 | Chenevez2012 |
Orbital period (Porb) [min] | ||
Porb determination method | ||
Thermonuclear X-ray burst | Short-B | Chenevez2012Wijnands2017Fiocchi2019Marino2019 |
Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
1.97E-09 | Degenaar2016 |
NH [x1022 cm-2] | 0.48±0.02 | Degenaar2016 |
E(B-V) [mag] | ||
Magnitude | V=17.71±0.02 | Baglio2016 |
Proposed companion | He rich companion? (optical spectra) |
Baglio2016 |
Tse2021 detect Millihertz QPOs with frequencies in the range 5-8 mHz, driven by thermonuclear burning. |
UV | ||
---|---|---|
Optical | Tentative He II λ4686 emission line | Baglio2016 |
X-ray | N VII (~0.5 keV) O VII (~0.57 keV), O VIII (~0.65 keV) reflection lines, F Kα (~6.4 keV) | Ludlam2016Degenaar2016 |
|
|||
---|---|---|---|
B=18.03 ± 0.03, V=17.71 ± 0.02,R=17.24 ± 0.03,17.03 ± 0.06, g=17.84 ± 0.05,r=17.38 ± 0.03,i=17.02 ± 0.03,J=15.79 ± 0.12,K=14.68 ± 0.26, (UVOT)b=17.22 ± 0.08,u=16.45 ± 0.06,uvw1=16.90 ± 0.07,uvm2=17.86 ± 0.12,uvw2=17.58 ± 0.08 |