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The X-ray transient XTE J1118+480: Multiwavelength observations of a low-state minioutburst
被引:115
|作者:
Hynes, RI
[1
]
Mauche, CW
Haswell, CA
Shrader, CR
Cui, W
Chaty, S
机构:
[1] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England
[2] Univ Calif Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[3] Open Univ, Dept Phys & Astron, Milton Keynes MK7 6AA, Bucks, England
[4] NASA, Goddard Space Flight Ctr, High Energy Astrophys Lab, Greenbelt, MD 20771 USA
[5] MIT, Space Res Ctr, Cambridge, MA 02139 USA
基金:
美国国家航空航天局;
关键词:
accretion;
accretion disks;
binaries : close;
stars : individual (XTE J1118+480);
ultraviolet : stars;
X-rays : stars;
D O I:
10.1086/312836
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We present multiwavelength observations of the newly discovered X-ray transient XTE J1118+480 obtained in the rising phase of the 2000 April outburst. This source is located at unusually high Galactic latitude and in a very low absorption line of sight. This made the first Extreme Ultraviolet Explorer (EUVE) spectroscopy of an X-ray transient outburst possible, Together with our Hubble Space Telescope, Rossi X-Ray Timing Explorer, and United Kingdom Infrared Telescope data, this gives unprecedented spectral coverage. We find the source in the low hard state. The flat IR-UV continuum appears to be a combination of optically thick disk emission and possibly synchrotron, while at higher energies (including; EUV), a typical low hard state power law is seen. EUVE observations reveal no periodic modulation, suggesting an inclination low enough that no obscuration by the disk rim occurs. We discuss the nature of the source and this outburst and conclude that it may be more akin to minioutbursts seen in GRO J0422+32 than to a normal X-ray transient outburst.
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页码:L37 / L40
页数:4
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