2010MNRAS.409..839C

Query : 2010MNRAS.409..839C

2010MNRAS.409..839C - Mon. Not. R. Astron. Soc., 409, 839-845 (2010/December-1)

Limits on the quiescent radio emission from the black hole binaries GRO J1655-40 and XTE J1550-564.

CALVELO D.E., FENDER R.P., RUSSELL D.M., GALLO E., CORBEL S., TZIOUMIS A.K., BELL M.E., LEWIS F. and MACCARONE T.J.

Abstract (from CDS):

We present the results of radio observations of the black hole binaries GRO J1655-40 and XTE J1550-564 in quiescence, with the upgraded Australia Telescope Compact Array. Neither system was detected. Radio flux density upper limits (3σ) of 26 µJy (at 5.5 GHz), 47 µJy (at 9 GHz) for GRO J1655-40 and 1.4 mJy (at 1.75 GHz), 27 µJy (at 5.5 GHz), 47 µJy (at 9 GHz) for XTE J1550-564 were measured. In conjunction with quasi-simultaneous Chandra X-ray observations (in the case of GRO J1655-40) and Faulkes Telescope optical observations (XTE J1550-564) we find that these systems provide the first evidence of relatively `radio-quiet' black hole binaries at low luminosities, indicating that the scatter observed in the hard state X-ray-radio correlation at higher luminosities may also extend towards quiescent levels.

Abstract Copyright: © 2010 The Authors. Journal compilation © 2010 RAS

Journal keyword(s): black hole physics - binaries: close - stars: individual: XTE J1550-564 - stars: individual: GRO J1655-40 - ISM: jets and outflows - X-rays: binaries

Simbad objects: 24

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Number of rows : 24
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 V* V518 Per HXB 04 21 42.7227473352 +32 54 26.939156184           M4.5V 670 0
2 1A 0620-00 HXB 06 22 44.5423857312 -00 20 44.290460544           K3V-K7V 1144 0
3 ICRF J082526.8-501038 QSO 08 25 26.8673494560 -50 10 38.484054768   20.94       ~ 139 1
4 V* MM Vel HXB 10 13 36.3431303106 -45 04 31.128938218           G5V-M0V 211 1
5 V* KV UMa HXB 11 18 10.7930420496 +48 02 12.314730120           K5V-M1V 865 0
6 V* BW Cir HXB 13 58 09.7227337579 -64 44 05.257858491           ~ 256 0
7 V* IL Lup HXB 15 47 08.2768672752 -47 40 10.284587760         15.624 ~ 532 1
8 V* V381 Nor HXB 15 50 58.6637920704 -56 28 35.258385000           K3III 1254 0
9 PKS 1613-586 rG 16 17 17.89125660 -58 48 07.8601409   18.23       ~ 156 1
10 [GHJ2008] 3 HXB 16 50 00.980 -49 57 43.60           K4V 422 0
11 V* V1033 Sco HXB 16 54 00.1423963019 -39 50 44.761701340       16.14   F3-6IV 1980 0
12 V* V821 Ara LXB 17 02 49.3876391280 -48 47 23.087954544         15.322 ~ 2237 0
13 V* V1228 Sco LXB 17 19 58.990 -31 45 01.11           ~ 122 1
14 PMN J1733-3722 Rad 17 33 15.1930935 -37 22 32.398009           ~ 56 1
15 2E 3938 HXB 17 43 54.7 -29 44 44           ~ 693 1
16 NAME XTE J17464-3213 LXB 17 46 15.59637 -32 14 00.8600           ~ 805 0
17 2MAXI J1753-013 LXB 17 53 28.2898766424 -01 27 06.256555272 15.30 16.73 16.46 16.15 15.64 ~ 384 0
18 2CXO J180112.3-254436 HXB 18 01 12.4783119670 -25 44 35.694663099           AV 417 1
19 V* V406 Vul HXB 18 58 41.49127200 +22 39 29.7746640           G5V-K0V 409 0
20 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2810 0
21 ICRF J193925.0-634245 Sy2 19 39 25.0245304992 -63 42 45.640373400   18.87 18.37 17.64   ~ 1332 2
22 HD 226868 HXB 19 58 21.6757355952 +35 12 05.784512688 9.38 9.72 8.91 8.42   O9.7Iabpvar 4590 0
23 V* QZ Vul HXB 20 02 49.5220407111 +25 14 10.631666444           K3V-K6V 432 0
24 V* V404 Cyg HXB 20 24 03.8247037434 +33 52 01.961154861           G9/K0III/V 1370 0

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