2 VARIABLE X-RAY SOURCES IN M31

被引:12
作者
COLLURA, A [1 ]
REALE, F [1 ]
PERES, G [1 ]
机构
[1] OSSERV ASTRON PALERMO,I-90134 PALERMO,ITALY
关键词
Galaxies: individual (M31); X-rays: binaries; X-rays: sources;
D O I
10.1086/168822
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have analyzed the entire set of Einstein observations of M31, consisting of five imaging proportional counter and nine high resolution imager observations, for variability of the X-ray sources. The time scales explored range up to ∼ 105 s, the maximum time span of individual observations. We detect variability above the adopted 99.73% significance level in two sources and derive constraints on their possible periodicity. The observed X-ray luminosities, the pattern of variability, and the optical identifications suggest the possibility that one of them is a low-mass X-ray binary and the other one a compact massive X-ray binary. We also discuss the analysis of the nonvariable sources and derive upper limits on the detectable variability of the various sources. The number of variable sources detected is in agreement with the expectations based on the features of intense Galactic X-ray sources and on the characteristics of the observations.
引用
收藏
页码:119 / 129
页数:11
相关论文
共 50 条
  • [21] Discovery and modelling of disc precession in the M31 X-ray binary Bo 158
    Barnard, R
    Foulkes, SB
    Haswell, CA
    Kolb, U
    Osborne, JP
    Murray, JR
    PROCEEDINGS OF THE X-RAY UNIVERSE 2005, VOLS 1 AND 2, 2006, 604 : 207 - +
  • [22] A Chandra Study of the Stellar X-Ray Emissivity of Globular Clusters in the M31 Bulge
    Xu, Xiao-jie
    Li, Zhiyuan
    ASTROPHYSICAL JOURNAL, 2018, 856 (01)
  • [23] Discovery of Periodic Dips in the Brightest Hard X-Ray Source of M31 with EXTraS
    Marelli, Martino
    Tiengo, Andrea
    De Luca, Andrea
    Salvetti, David
    Saronni, Luca
    Sidoli, Lara
    Paizis, Adamantia
    Salvaterra, Ruben
    Belfiore, Andrea
    Israel, Gianluca
    Haberl, Frank
    D'Agostino, Daniele
    ASTROPHYSICAL JOURNAL LETTERS, 2017, 851 (02)
  • [24] Identifying new X-ray binary candidates in M31 using random forest classification
    Arnason, R. M.
    Barmby, P.
    Vulic, N.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 492 (04) : 5075 - 5088
  • [25] Bright X-ray transients in M31:: 2004 July XMM-Newton observations
    Trudolyubov, Sergey
    Priedhorsky, William
    Cordova, France
    ASTROPHYSICAL JOURNAL, 2006, 645 (01) : 277 - 282
  • [26] Optical novae: the major class of supersoft X-ray sources in M 31
    Pietsch, W
    Fliri, J
    Freyberg, MJ
    Greiner, J
    Haberl, F
    Riffeser, A
    Sala, G
    ASTRONOMY & ASTROPHYSICS, 2005, 442 (03) : 879 - 894
  • [27] Swift observations of the ultraluminous X-ray source XMMU J004243.6+412519 in M31
    Esposito, P.
    Motta, S. E.
    Pintore, F.
    Zampieri, L.
    Tomasella, L.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 428 (03) : 2480 - 2488
  • [28] A systematic study of low-mass X-ray binaries in the M31 globular cluster system
    Peacock, Mark B.
    Maccarone, Thomas J.
    Kundu, Arunav
    Zepf, Stephen E.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 407 (04) : 2611 - 2624
  • [29] A potential supernova remnant-X-ray binary association in M31
    Williams, BF
    Barnard, R
    Garcia, MR
    Kolb, U
    Osborne, JP
    Kong, AKH
    ASTROPHYSICAL JOURNAL, 2005, 634 (01) : 365 - 375
  • [30] REINSTATING THE M31 X-RAY SYSTEM RX J0042.3+4115 AS A BLACK HOLE X-RAY BINARY AND COMPELLING EVIDENCE FOR AN EXTENDED CORONA
    Barnard, R.
    Garcia, M. R.
    Murray, S. S.
    ASTROPHYSICAL JOURNAL, 2011, 743 (02)