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
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