RA Dec
|
ℓ b
|
| Location in Globular Cluster | Terzan 2 | |
|---|---|---|
| Type of accretor | NS | Persistent |
|
Distance [kpc] (other distances) Gaia [kpc] |
7.753
+0.332-0.318 6.6+2.8-4 |
Baumgardt2021 Harris2010Valenti2010Kuulkers2003Galloway2020Galloway2008Chelovekov2011Chelovekov2017 Arnason2021 |
| z [kpc] | 0.31 | Baumgardt2021 |
| Orbital period (Porb) [min] | ||
| Porb determination method | ||
| Thermonuclear X-ray burst | Short-B | Swank1977Kuulkers2003 |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
5.74E-10 | Lin2018 |
| NH [x1022 cm-2] | 1.1 | Kashyap2022 |
| E(B-V) [mag] | 1.87±0.19 | Harris2010Valenti2010 |
| Magnitude | ||
| Proposed companion |
| Radio flux < 0.28 mJy (6 cm; Grindlay1986). Altamirano2008b proposed an orbital periodicity of ~90 days (see also Tarana2018). |
| UV | ||
|---|---|---|
| Optical | ||
| X-ray | Weak Fe emission line (~6.4 keV) | Barret2000 |
|
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|---|---|---|---|
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