2012MNRAS.423.2656R


Query : 2012MNRAS.423.2656R

2012MNRAS.423.2656R - Mon. Not. R. Astron. Soc., 423, 2656-2667 (2012/July-1)

The black hole candidate XTE J1752-223 towards and in quiescence: optical and simultaneous x-ray–radio observations.

RATTI E.M., JONKER P.G., MILLER-JONES J.C.A., TORRES M.A.P., HOMAN J., MARKOFF S., TOMSICK J.A., KAARET P., WIJNANDS R., GALLO E., OZEL F., STEEGHS D.T.H. and FENDER R.P.

Abstract (from CDS):

We present optical, X-ray and radio observations of the black hole transient (BHT) XTE J1752-223 towards and in quiescence. Optical photometry shows that the quiescent magnitude of XTE J1752-223 is fainter than 24.4 mag in the i' band. A comparison with measurements of the source during its 2009–2010 outburst shows that the outburst amplitude is more than 8 mag in the i' band. Known X-ray properties of the source combined with the faintness of the quiescence optical counterpart and the large outburst optical amplitude point towards a short orbital-period system (Porb ≲ 6.8 h) with an M type (or later) mass donor, at a distance of 3.5 ≲ d ≲ 8 kpc. Simultaneous X-ray and radio data were collected with Chandra and the Expanded Very Large Array (EVLA), allowing constraints to be placed on the quiescent X-ray and radio flux of XTE J1752-223. Furthermore, using data covering the final stage of the outburst decay, we investigated the low-luminosity end of the X-ray–radio correlation for this source and compared it with other BHTs. We found that XTE J1752-223 adds to the number of outliers with respect to the `standard' X-ray–radio luminosity relation. Furthermore, XTE J1752-223 is the second source, after the BHT H1743-322, that shows a transition from the region of the outliers towards the `standard' correlation at low luminosity. Finally, we report on a faint, variable X-ray source we discovered with Chandra at an angular distance of ∼2.9 arcsec to XTE J1752-223 and at a position angle consistent with that of the radio jets previously observed from the BHT. We discuss the possibility that we detected X-ray emission associated with a jet from XTE J1752-223.

Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society2012 RAS

Journal keyword(s): accretion, accretion discs - binaries: general - stars: individual: XTE J1752-223 - X-rays: binaries

Simbad objects: 38

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Number of rows : 38
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 V* V518 Per HXB 04 21 42.7227473352 +32 54 26.939156184 13.00 13.50 13.2     M4.5V 638 1
2 1A 0620-00 HXB 06 22 44.5423857312 -00 20 44.290460544 10.60 11.40 11.2     K3V-K7V 1073 0
3 V* KV UMa HXB 11 18 10.7930420496 +48 02 12.314730120     12.25     K5V-M1V 769 0
4 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4121 2
5 V* BW Cir HXB 13 58 09.700 -64 44 05.80 17.90 18.00 16.9     ~ 217 1
6 QSO B1404+286 BLL 14 07 00.3941769384 +28 27 14.692128372   16.13 15.35 10.29   ~ 731 2
7 V* BR Cir HXB 15 20 40.85 -57 10 00.1   21.4 21.4     ~ 748 1
8 V* IL Lup HXB 15 47 08.2768672752 -47 40 10.284587760     11.96     ~ 453 1
9 V* V381 Nor HXB 15 50 58.6637920704 -56 28 35.258385000   17.95 16.6     K3III 1103 0
10 V* V818 Sco LXB 16 19 55.0692669024 -15 38 25.017666540 11.60 12.40 11.1     Oev 1580 0
11 [GHJ2008] 3 HXB 16 50 00.980 -49 57 43.60     11.89     K4V 370 0
12 V* V1033 Sco HXB 16 54 00.137 -39 50 44.90   15.20 14.2 16.14   F5IV 1800 1
13 MAXI J1659-152 LXB 16 59 01.680 -15 15 28.73           ~ 223 0
14 V* V821 Ara HXB 17 02 49.3876391280 -48 47 23.087954544 16.20 16.30 15.5     ~ 1952 0
15 [KRL2007b] 222 LXB 17 09 07.61 -36 24 25.7           ~ 245 1
16 V* V1228 Sco LXB 17 19 58.990 -31 45 01.11           ~ 110 1
17 NAME Great Annihilator LXB 17 43 54.83 -29 44 42.6           ~ 659 1
18 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 13204 0
19 NAME XTE J17464-3213 LXB 17 46 15.59637 -32 14 00.8600           ~ 677 0
20 [IBR2011] J1751-1950 Rad 17 51 41.3437536 -19 50 47.504157           ~ 14 0
21 CXOU J175215.0-222010 X 17 52 15.06 -22 20 10.9           ~ 1 0
22 XTE J1752-223 LXB 17 52 15.090 -22 20 32.36           ~ 186 0
23 CXOU J175215.1-222035 X 17 52 15.19 -22 20 35.4           ~ 1 0
24 CXOU J175215.4-222023 X 17 52 15.46 -22 20 23.9           ~ 1 0
25 CXOU J175215.4-222036 X 17 52 15.49 -22 20 37.0           ~ 1 0
26 CXOU J175215.9-222001 X 17 52 16.010 -22 20 02.25           ~ 1 0
27 2MAXI J1753-013 LXB 17 53 28.2898766424 -01 27 06.256555272 15.30 16.73 16.46 16.15 15.64 ~ 330 0
28 PMN J1755-2232 Rad 17 55 26.284538 -22 32 10.61562           ~ 31 0
29 2XMM J180112.4-254436 LXB 18 01 12.40 -25 44 36.1           ~ 376 1
30 V* V4641 Sgr HXB 18 19 21.6343259256 -25 24 25.849595952     13.654   13.092 B9III 437 1
31 QSO J1820-2528 QSO 18 20 57.84869182 -25 28 12.5836842   18.56       ~ 90 0
32 V* V406 Vul HXB 18 58 41.580 +22 39 29.40 15.00 15.65 15.31     G5V-K0V 348 0
33 [KRL2007b] 353 HXB 19 08 53.080 +09 23 04.84     15.80     ~ 101 0
34 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2464 0
35 HD 226868 HXB 19 58 21.6757355952 +35 12 05.784512688 9.38 9.72 8.91 8.42   O9.7Iabpvar 4140 0
36 V* QZ Vul HXB 20 02 49.58 +25 14 11.3   19.64 18.2     K3V-K6V 408 0
37 V* V404 Cyg HXB 20 24 03.8254458776 +33 52 01.962185735           G9/K0III/V 1192 0
38 NAME Galactic Bulge reg ~ ~           ~ 3938 0

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2022.10.06-20:46:32

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