RA Dec
|
ℓ b
|
Location in Globular Cluster | ||
---|---|---|
Type of accretor | NS | Persistent |
Distance [kpc] (other distances) Gaia [kpc] |
Gaia 2.1
+0.7-1.2 2.6+0.8-1.3 |
Arnason2021 Mukai2001Jonker2003aHakala1998Hakala2005 BailerJones2018 |
z [kpc] | 1.53 | Arnason2021 |
Orbital period (Porb) [min] | 111.04 | Morris1990 |
Porb determination method | Optical eclipse | |
Thermonuclear X-ray burst | short-B | Hakala2005Mukai2001 |
Peak X-ray flux [erg s-1 cm-2] (2 - 10 keV) |
4.19E-12 | Jonker2003a |
NH [x1022 cm-2] | 0.15±0.03 | Jonker2003a |
E(B-V) [mag] | ||
Magnitude | R=19.4 | Morris1990 |
Proposed companion |
Manson2012 report an upper limit of the change of the orbital period of |P| < 4.2E-11. Optical bursts were suggested to arise from reprocessed type I X-ray bursts in the companion star (Hynes2004c) or in the accretion disc (Manson2012). |
UV | ||
---|---|---|
Optical | Hα, Hβ, He II λ4686 emission lines; He I and Ca II absorption lines | Morris1990 |
X-ray | Evidence for emission lines at ~0.5 keV and ~0.65 keV (N VII, O VIII Lyα ?) | Hakala2005 |
|
|||
---|---|---|---|
R~19.4, B=19.37, G=19.53±0.01, BP=19.52±0.05, RP=19.47±0.05, u=19.527±0.028, g=19.546±0.012, r=19.705±0.016, i=19.845±0.027, z=19.911±0.091 |
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