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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.
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页码:1563 / 1569
页数:7
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