A search for the optical/infrared counterpart of the anomalous X-ray pulsar 1E 1841-045

被引:11
作者
Mereghetti, S
Mignani, RP
Covino, S
Chaty, S
Israel, GL
Neuhäuser, R
Plana, H
Stella, L
机构
[1] CNR, Ist Fis Cosm, I-20133 Milan, Italy
[2] ESO, D-85748 Garching, Germany
[3] Osservatorio Astron Merate, I-22055 Merate, LC, Italy
[4] Open Univ, Dept Phys & Astron, Milton Keynes MK7 6AA, Bucks, England
[5] Osservatorio Astron Roma, I-00040 Rome, Italy
[6] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
[7] Observ Astron Nacl, Ensenada, Baja California, Mexico
关键词
pulsars : individual : 1E 1841-045; X-rays : stars;
D O I
10.1046/j.1365-8711.2001.03988.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have carried out a search for the optical and infrared counterpart of the anomalous X-ray pulsar 1E 1841-045, which is located at the centre of the supernova remnant Kes 73. We present the first deep optical and infrared images of the field of 1E 1841-045, as well as optical spectroscopy results that exclude the brightest objects in the error circle as possible counterparts. A few of the more reddened objects in this region can be considered as particularly interesting candidates, in consideration of the distance and absorption expected from the association with Kes 73. The strong interstellar absorption in the direction of the source does not allow us to exclude completely the presence of main-sequence massive companions.
引用
收藏
页码:143 / 148
页数:6
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