RA Dec
|
ℓ b
|
| Location in Globular Cluster | ||
|---|---|---|
| Type of accretor |
NS AMXP (163.65 Hz / 6.11 ms) |
Persistent (Quasi-persistent) Strohmayer2017 |
|
Distance [kpc] (other distances) Gaia [kpc] |
7.3±0.5 (He)
3.4-1.7+6.4 |
Keek2017 Degenaar2013a BailerJones2018 |
| z [kpc] | -1.57 | Keek2017 |
| Orbital period (Porb) [min] | 37.9701±0.0002 | Strohmayer2018 |
| Porb determination method | X-ray pulsation | |
| Thermonuclear X-ray burst | IB SB |
Degenaar2012a Negoro2015 |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
5.53E-11 | Keek2017 |
| NH [x1022 cm-2] | 0.26 | Degenaar2017 |
| E(B-V) [mag] | ||
| Magnitude | g'=20.23±0.16 | HernandezSantisteban2019 |
| Proposed companion | He;
CO or O-Ne-Mg WD (Constraints on the donor mass and radius; X-ray spectral modelling) |
Strohmayer2018 VandenEijnden2018 |
| UV | ||
|---|---|---|
| Optical | Featureless | HernandezSantisteban2019 |
| X-ray | Fe Kα (~6 keV) Emission and absorption lines in the Fe K band (7-10 keV) Emission line at 1 keV (Fe-L complex) O emission line (0.63-0.69 keV) Absorption line at 3.4 keV (Ca or Ti) |
Strohmayer2017Keek2017 Degenaar2013a IntZand2019Degenaar2013a VandenEijnden2018Bult2021 Bult2021 |
|
|||
|---|---|---|---|
| UVW2=20.10±0.05, UVM2=20.40±0.15, UVW1=20.03±0.08, U=19.85±0.39, B=20.30±1.69, g'_1=20.23±0.16, g'_2=20.29±0.13, r'_1=20.30±0.17, r'_2=20.12±0.10, i'_1=20.37±0.19, i'_2=20.05±0.12, J_1=20.54±0.08, J_2=20.84±0.04, J_3=23.39±0.18, H_1=20.63±0.08, H_2=20.44±0.05, H_3=22.96±0.44, Ks_1=20.98±0.11, Ks_2=20.78±0.10, Ks_3=22.93±0.39 (different telescopes and epochs). | |||