Accurate positions for the ultraluminous X-ray sources NGC 7319-X4 and NGC 5474-X1 and limiting magnitudes for their optical counterparts

被引:2
|
作者
Heida, M. [1 ,2 ]
Jonker, P. G. [1 ,2 ,3 ]
Torres, M. A. P. [1 ,3 ]
Mineo, S. [3 ]
机构
[1] SRON Netherlands Inst Space Res, NL-3584 CA Utrecht, Netherlands
[2] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, NL-6500 GL Nijmegen, Netherlands
[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
galaxies: individual: NGC 5474; galaxies: individual: NGC 7319; X-rays: binaries; X-rays: individual: NGC 5474-X1; X-rays: individual: NGC 7319-X4; SUPERMASSIVE BLACK-HOLES; SKY SURVEY; GALAXIES; SUPERNOVAE; EMISSION; MASS; CALIBRATION; BINARIES; REDSHIFT; SYSTEMS;
D O I
10.1111/j.1365-2966.2012.21370.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we report accurate Chandra positions for two ultraluminous X-ray sources (ULXs): NGC 7319-X4 at Right Ascension (RA) = 339029 17(2), Declination (Dec.) = 33974 76(2) and NGC 5474-X1 at RA = 211248 59(3), Dec. = 53635 84(3). We perform bore-sight corrections on the Chandra X-ray satellite observations of these sources to get these accurate positions of the X-ray sources and match these positions with archival optical data from the Wide Field Planetary Camera 2 (WFPC2) onboard the Hubble Space Telescope. We do not find the optical counterparts; the limiting absolute magnitudes of the observations in the WFPC2 standard magnitude system are B=-7.9, V=-8.7 and I=-9.3 for NGC 7319-X4 and U=-6.4 for NGC 5474-X1. We report on the X-ray spectral properties and find evidence for X-ray variability in NGC 5474-X1. Finally, we briefly discuss several options for the nature of these ULXs.
引用
收藏
页码:1563 / 1569
页数:7
相关论文
共 50 条
  • [41] X-ray Sources Population in NGC 1559
    Nazri, Nurnabilah
    Annuar, Adlyka
    JURNAL KEJURUTERAAN, 2020, 3 (01): : 7 - 14
  • [42] X-RAY SOURCES AND THEIR OPTICAL COUNTERPARTS IN THE GALACTIC GLOBULAR CLUSTER M12 (NGC 6218)
    Lu, Ting-Ni
    Kong, Albert K. H.
    Bassa, Cees
    Verbunt, Frank
    Lewin, Walter H. G.
    Anderson, Scott F.
    Pooley, David
    ASTROPHYSICAL JOURNAL, 2009, 705 (01) : 175 - 183
  • [43] A Long-Term Study of Ultraluminous X-ray Sources in NGC 891
    Earley, Nicholas M.
    Dwarkadas, Vikram V.
    Cirillo, Victoria
    UNIVERSE, 2022, 8 (01)
  • [44] A deep search for faint Chandra X-ray sources, radio sources, and optical counterparts in NGC 6752
    Cohn, Haldan N.
    Lugger, Phyllis M.
    Zhao, Yue
    Tudor, Vlad
    Heinke, Craig O.
    Cool, Adrienne M.
    Anderson, Jay
    Strader, Jay
    Miller-Jones, James C. A.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 508 (02) : 2823 - 2847
  • [45] X-ray reverberation models of the disc wind in ultraluminous X-ray source NGC 5408 X-1
    Luangtip, W.
    Chainakun, P.
    Loekkesee, S.
    Deesamer, C.
    Ngonsamrong, T.
    Sintusiri, T.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 507 (04) : 6094 - 6107
  • [46] NGC 7793 P9: An Ultraluminous X-Ray Source Evolved from a Canonical Black Hole X-Ray Binary
    Hu, Chin-Ping
    Kong, Albert K. H.
    Ng, C. -Y.
    Li, K. L.
    ASTROPHYSICAL JOURNAL, 2018, 864 (01)
  • [47] Chandra monitoring observations of the ultraluminous X-ray source NGC 5204 X-1
    Roberts, T. P.
    Kilgard, R. E.
    Warwick, R. S.
    Goad, M. R.
    Ward, M. J.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 371 (04) : 1877 - 1890
  • [48] THE X-RAY POINT-SOURCE POPULATION OF NGC 1365: THE PUZZLE OF TWO HIGHLY-VARIABLE ULTRALUMINOUS X-RAY SOURCES
    Strateva, Iskra V.
    Komossa, S.
    ASTROPHYSICAL JOURNAL, 2009, 692 (01) : 443 - 458
  • [49] Towards a dynamical mass of the ultraluminous X-ray source NGC 5408 X-1
    Cseh, D.
    Grise, F.
    Kaaret, P.
    Corbel, S.
    Scaringi, S.
    Groot, P.
    Falcke, H.
    Kording, E.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 435 (04) : 2896 - 2902
  • [50] The ultraluminous X-ray source NGC 1313 X-2 -: Its optical counterpart and environment
    Grise, F.
    Pakull, M. W.
    Soria, R.
    Motch, C.
    Smith, I. A.
    Ryder, S. D.
    Bottcher, M.
    ASTRONOMY & ASTROPHYSICS, 2008, 486 (01): : 151 - 163