RA Dec
|
ℓ b
|
Location in Globular Cluster | NGC 2808 | |
---|---|---|
Type of accretor |
NS AMXP (339.97 Hz / 2.94 ms) |
Transient Sanna2017 |
Distance [kpc] (other distances) |
10.060
+0.112-0.111 |
Baumgardt2021 Harris2010Watkins2015 |
z [kpc] | -1.95 | Baumgardt2021 |
Orbital period (Porb) [min] | 44.332218±0.000007 | Sanna2017 |
Porb determination method | X-ray pulsation | |
Thermonuclear X-ray burst | IB |
Nakajima2020 |
Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
1.37E-10 | Sanna2017 |
NH [x1022 cm-2] | 0.25±0.01 | Sanna2017 |
E(B-V) [mag] | 0.22±0.02 | Harris2010 |
Magnitude | ||
Proposed companion |
No radio counterpart was detected down to a 5σ upper limit of 70 μJy during the 2016 outburst (5.5 and 9 GHz; Tudor2016). NICER observations performed in July 2021 suggested that the source never returned to quiescence since it was first discovered in 2016 (Ng2021b), although it briefly dipped in flux around June 2019 (Parikh2019). |
UV | ||
---|---|---|
Optical | ||
X-ray | Fe Kα (6.5 - 6.6 keV) | Sanna2017 |
|
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