2018MNRAS.474...69A


C.D.S. - SIMBAD4 rel 1.7 - 2021.04.19CEST15:37:13

2018MNRAS.474...69A - Mon. Not. R. Astron. Soc., 474, 69-76 (2018/February-2)

Selection effects on the orbital period distribution of low-mass black hole X-ray binaries.

ARUR K. and MACCARONE T.J.

Abstract (from CDS):

We investigate the lack of observed low-mass black hole binary systems at short periods(<4 h) by comparing the observed orbital period distribution of 17 confirmed low-mass black hole X-ray binaries (BHXBs) with their implied period distribution after correcting for the effects of extinction of the optical counterpart, absorption of the X-ray outburst and the probability of detecting a source in outburst. We also draw samples from two simple orbital period distributions and compare the simulated and observed orbital period distributions. We predict that there are >200 and <3000 binaries in the Galaxy with periods between 2 and 3 h, with an additional ≃600 objects between 3 and 10 h.

Abstract Copyright: © 2017 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): stars: black holes - X-rays: binaries

CDS comments: Table 1: V22107 Oph is a misprint for V2107 Oph.

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 - 2021
#notes
1 V* V518 Per HXB 04 21 42.7231318463 +32 54 26.936934166 13.00 13.50 13.2     M4.5V 626 1
2 1A 0620-00 HXB 06 22 44.5420315454 -00 20 44.289428950 10.60 11.40 11.2     K3V-K7V 1052 0
3 V* MM Vel HXB 10 13 36.4107940553 -45 04 32.555813596   14.84 14.71     G5V-M0V 187 0
4 V* KV UMa HXB 11 18 10.7922353051 +48 02 12.319175505     12.25     K5V-M1V 737 0
5 V* GU Mus HXB 11 26 26.5947467816 -68 40 32.888148788           K3V-K7V 677 1
6 MAXI J1305-704 XB* 13 06 55.300 -70 27 05.11           ~ 46 0
7 V* BW Cir HXB 13 58 09.700 -64 44 05.80 17.90 18.00 16.9     ~ 202 1
8 V* IL Lup HXB 15 47 08.2766679321 -47 40 10.284971214     11.96     ~ 426 1
9 V* V381 Nor HXB 15 50 58.6520652623 -56 28 35.309070422   17.95 16.6     K3III 1062 0
10 [GHJ2008] 3 HXB 16 50 00.980 -49 57 43.60     11.89     K4V 358 0
11 V* V1033 Sco HXB 16 54 00.137 -39 50 44.90   15.20 14.2 16.14   F5IV 1751 1
12 MAXI J1659-152 LXB 16 59 01.680 -15 15 28.73           ~ 199 0
13 V* V821 Ara HXB 17 02 49.3810714542 -48 47 23.163091737 16.20 16.30 15.5     ~ 1826 0
14 V* V2107 Oph HXB 17 08 14.520 -25 05 30.15   16.50 15.9     K3V-K7V 213 1
15 2MAXI J1753-013 LXB 17 53 28.2897263704 -01 27 06.256526637 15.30 16.73 16.46 16.15 15.64 ~ 302 0
16 V* V4641 Sgr HXB 18 19 21.6342721789 -25 24 25.849323550     13.654   13.092 B9III 407 1
17 MAXI J1836-194 XB* 18 35 43.440 -19 19 10.48           ~ 113 0
18 V* V406 Vul HXB 18 58 41.580 +22 39 29.40 15.00 15.65 15.31     G5V-K0V 326 0
19 MAXI J1910-057 LXB 19 10 22.80 -05 47 55.9           ~ 54 0
20 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2361 0
21 V* V1408 Aql LXB 19 59 24.0077707935 +11 42 29.856991417 18.40 18.97 18.95 18.70 18.66 ~ 174 0
22 V* QZ Vul HXB 20 02 49.58 +25 14 11.3   19.64 18.2     K3V-K6V 400 0
23 V* V404 Cyg HXB 20 24 03.820 +33 52 01.90 14.50 14.20 12.7     K0IV 1125 0
24 M 15 GlC 21 29 58.33 +12 10 01.2   3       ~ 2952 0

    Equat.    Gal    SGal    Ecl

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2021.04.19-15:37:13

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