RA Dec
|
ℓ b
|
| Location in Globular Cluster | NGC 6293 | |
|---|---|---|
| Type of accretor | NS | Transient |
|
Distance [kpc] (other distances) |
9.192
+0.282-0.274 |
Baumgardt2021 Harris1996Harris2010Jonker2004aLee2006Galloway2020 |
| z [kpc] | 1.27 | Baumgardt2021 |
| Orbital period (Porb) [min] | ||
| Porb determination method | ||
| Thermonuclear X-ray burst | Short-B | Cocchi1998 |
| Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
9.10E-10 | Ludlam2017 |
| NH [x1022 cm-2] | 0.29±0.01 | Degenaar2013 |
| E(B-V) [mag] | 0.36±0.04 | Harris2010 |
| Magnitude | R=20.5±0.1 qR=22.24±0.03 |
Jonker2004a |
| Proposed companion | O/Ne WD (X-ray spectral modelling) |
Jonker2003 |
| Although the orbital period is unknown, Jonker2003 found an excess emission at ~0.6 keV that makes the source an UCXB candidate. |
| UV | ||
|---|---|---|
| Optical | ||
| X-ray | Excess emission at 0.6 keV (O and/or Fe, enhanced Ne/O) Fe Kα (~6.5 keV) |
Jonker2003 Ludlam2017 |
|
|||
|---|---|---|---|
| R=20.5±0.1, R=22.24±0.03 (qui), qmV < 20.5, V=17.9 | |||
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