UltraCompCAT A Catalogue of Ultra-Compact and Short Orbital Period X-ray Binaries

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ID# 26

NGC 6652 B

CXOGLB J183544.5-325939

Candidate UCXB

RA                 Dec    

[hh:mm:ss.ss]          [dd:mm:ss.ss]

18:35:44.54  -32:59:38.97

                     [ICRS]

ℓ                      b

[deg]                            [deg]

001.529081  -11.374830

Year of discovery: 1998

(Deutsch1998Heinke2001)

Basic data

Location in Globular Cluster NGC 6652
Type of accretor NS Transient
Distance [kpc]
(other distances)
9.464 +0.139-0.137
Baumgardt2021
Kuulkers2003Harris2010Chelovekov2011
z [kpc] -1.87 Baumgardt2021
Orbital period (Porb) [min]
Porb determination method
Thermonuclear X-ray burst Short-B Intzand1998
Peak X-ray flux [erg s-1 cm-2]
(2 - 10 keV)
7.52E-13 Stacey2012
NH [x1022 cm-2] 0.05 Coomber2011
E(B-V) [mag] 0.09±0.01 Harris2010
Magnitude B = 20.4 Deutsch1998
Proposed companion - MS (not compatible with Porb) or degenerate (not compatible with colors).
- Early to mid G-type star.
(- Geometry and observed parameter's arguments.
- Optical spectrum)
Heinke2001

Paduano2021


NOTES

NGC 6652 B can only be separated from NGC 6652 A (XB 1832-330) by Chandra; then, properties such as bursts and activity (transient or persistent), have to be considered carefully, since they could belong to either source.
Deutsch1998 identified an optical counterpart with NGC 6652 A and Deutsch2000 estimated an orbital period of 43.6 (+/-0.6) min, based in optical modulation (HST). But later, Heinke2001 associated that counterpart with NGC 6652 B from Chandra data.
Engel2012 obtained a light curve that shows a lot of flickering and suggested that the orbital period reported by Deutsch2000 is spurious (this was also suggested by Heinke2001).
Radio flux density = 79.2 ± 2.2 μJy (10 GHz; Paduano2021).

Spectral data

UV
Optical H and He emission features (changing to absorption in ~2 hours), G-band, and metallic absorption lines (Fe, Mg, Na, O). Paduano2021
X-ray

Peak Optical/NIR magnitudes

If the system is transient, quiescent magnitudes are indicated with a "q" superindex
Deutsch1998 Paduano2021 Skottfelt2015
B = 20.4, V > 17.7, I = 18.72
Aladin finding chart
Scroll to zoom. Set survey image in "Manage layers"
Default image: DSS2 Red
NGC 6652 B in Simbad

References to finding charts

Heinke2001Deutsch1998Engel2012Skottfelt2015



This research has made use of NASA's Astrophysics Data System (ADS) and the SIMBAD database operated at CDS (Strasbourg, France)
Please acknowledge the use of this catalogue in any published work you derive from it.

Last modified: 09 May 2023.