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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