Near-infrared, optical, and X-ray observations of the anomalous X-ray pulsar 4U 0142+61

被引:17
作者
Morii, M
Kawai, N
Kataoka, J
Yatsu, Y
Kobayashi, N
Terada, H
机构
[1] Japan Aerosp Explorat Agcy, Tsukuba Space Ctr, ISS Sci Project Off, MAXI Grp, Tsukuba, Ibaraki 3058505, Japan
[2] Tokyo Inst Technol, Meguro Ku, Tokyo 1528551, Japan
[3] Univ Tokyo, Astron Inst, Mitaka, Tokyo 1810015, Japan
[4] Natl Astron Observ, Subaru Telescope, Hilo, HI 96720 USA
来源
YOUNG NEUTRON STARS AND SUPERNOVA REMNANTS | 2005年 / 35卷 / 06期
关键词
neutron star; anomalous X-ray pulsar; magnetar;
D O I
10.1016/j.asr.2005.04.051
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
We present results from the simultaneous observations of an anomalous X-ray pulsar (AXP) 4U 0142 + 61 on Sep. 2003. We used RXTE, Subaru, and UH88 telescopes to cover X-ray, near-infrared (NIR) (JHK'), and optical (BVRI) bands, respectively. We obtained a simultaneous broadband spectrum for the first time among AXPs. We found NIR excess in the spectrum, which may be another component different from the optical one. We also found a R band dip. We discuss the broadband spectrum covering the optical and X-ray bands in the framework of a self absorbed synchrotron emission from the magnetosphere of magnetar. We also discuss about the R band dip feature, which could put a restriction on the emission models of magnetars. (c) 2005 Published by Elsevier Ltd on behalf of COSPAR.
引用
收藏
页码:1177 / 1180
页数:4
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