2011MNRAS.411..337D


C.D.S. - SIMBAD4 rel 1.7 - 2021.04.18CEST11:50:24

2011MNRAS.411..337D - Mon. Not. R. Astron. Soc., 411, 337-348 (2011/February-2)

A global study of the behaviour of black hole X-ray binary discs.

DUNN R.J.H., FENDER R.P., KORDING E.G., BELLONI T. and MERLONI A.

Abstract (from CDS):

We investigate the behaviour of the accretion discs in the outbursts of the low-mass black hole X-ray binaries (BHXRBs), an overview of which we have presented previously. Almost all of the systems in which there are sufficient observations in the most-disc-dominated states show a variation in the disc luminosity with temperature close to L ∝ T4. This in turn implies that in these states, the disc radius, Rin, and the colour correction factor, fcol, are almost constant. Deviations away from the T4 law are observed at the beginning and end of the most-disc-dominated states, during the intermediate states. Although these could be explained by an inward motion of the accretion disc, they are more likely to be the result of an increase in the value of fcol as the disc fraction decreases. By comparing the expected and observed disc luminosities, we place approximate limits on the allowed distances and masses of the BHXRB system. In a number of cases, the measured distances and masses of the BHXRB system indicate that it is possible that the black hole may be spinning.

Abstract Copyright: 2010 The Authors Monthly Notices of the Royal Astronomical Society2010 RAS

Journal keyword(s): accretion, accretion discs - binaries: general - ISM: jets and outflows - X-rays: binaries

Simbad objects: 28

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Number of rows : 28

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 X LMC X-3 HXB 05 38 56.6325045489 -64 05 03.321118015   17 17.2     B2.5Ve 637 0
2 X LMC X-1 HXB 05 39 38.8285930597 -69 44 35.533031148   14.8 14.5     O8(f)p 576 2
3 V* KV UMa HXB 11 18 10.7922353051 +48 02 12.319175505     12.25     K5V-M1V 737 0
4 V* BW Cir HXB 13 58 09.700 -64 44 05.80 17.90 18.00 16.9     ~ 202 1
5 V* IL Lup HXB 15 47 08.2766679321 -47 40 10.284971214     11.96     ~ 426 1
6 V* V381 Nor HXB 15 50 58.6520652623 -56 28 35.309070422   17.95 16.6     K3III 1062 0
7 X Nor X-1 LXB 16 34 01.610 -47 23 34.80           ~ 438 0
8 [GHJ2008] 3 HXB 16 50 00.980 -49 57 43.60     11.89     K4V 358 0
9 V* V1033 Sco HXB 16 54 00.137 -39 50 44.90   15.20 14.2 16.14   F5IV 1751 1
10 V* V821 Ara HXB 17 02 49.3810714542 -48 47 23.163091737 16.20 16.30 15.5     ~ 1826 0
11 SAX J1711.6-3808 XB* 17 11 37.1 -38 07 06           ~ 37 0
12 V* V1228 Sco LXB 17 19 58.990 -31 45 01.11           ~ 109 1
13 AX J1740.1-3102 X 17 40 09.000 -31 02 24.00           ~ 38 1
14 V* V2606 Oph CV* 17 42 40.030 -27 44 52.70     23.2     ~ 119 0
15 NAME XTE J17464-3213 LXB 17 46 15.59637 -32 14 00.8600           ~ 631 0
16 AX J1748.0-2829 LXB 17 48 05.060 -28 28 25.80     13.60     ~ 175 0
17 RX J1749.8-3312 LXB 17 49 48.940 -33 12 11.60           ~ 49 0
18 INTREF 866 LXB 17 55 28.6 -32 28 39     10.79     ~ 40 0
19 2XMM J180112.4-254436 LXB 18 01 12.40 -25 44 36.1           ~ 366 1
20 [KRL2007b] 312 LXB 18 17 43.537 -33 01 07.80           ~ 143 0
21 V* V4641 Sgr HXB 18 19 21.6342721789 -25 24 25.849323550     13.654   13.092 B9III 407 1
22 V* V406 Vul HXB 18 58 41.580 +22 39 29.40 15.00 15.65 15.31     G5V-K0V 326 0
23 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2361 0
24 HD 226868 HXB 19 58 21.6758193269 +35 12 05.782512305 9.38 9.72 8.91 8.42   O9.7Iabpvar 3997 0
25 V* V1408 Aql LXB 19 59 24.0077707935 +11 42 29.856991417 18.40 18.97 18.95 18.70 18.66 ~ 174 0
26 INTREF 1012 LXB 20 12 37.7593213138 +38 11 00.771841820     21.33     ~ 62 0
27 V* V404 Cyg HXB 20 24 03.820 +33 52 01.90 14.50 14.20 12.7     K0IV 1125 0
28 NAME Galactic Ridge ? ~ ~           ~ 444 1

    Equat.    Gal    SGal    Ecl

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