The radio counterpart of the X-ray pulsar wind nebula in the SNR G0.9+0.1

被引：0
|
作者：
Dubner, G [1 ]
Giacani, E
Decourchelle, A
机构：
[1] Inst Astron & Space Phys, Buenos Aires, DF, Argentina
[2] CEA Saclay, Serv Astrophys, Saclay, France
来源：
PROCEEDINGS OF THE X-RAY UNIVERSE 2005, VOLS 1 AND 2 | 2006年 / 604卷
关键词：
X-rays; radio continuum; supernova remnants; G0.9+0.1;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We report on new radio observations of the central nebula in the SNR G0.9+0.1 at 4.8 GHz and 8.6 GHz. These data unveil a highly clumpy structure of the radio nebula. Most of the radio features are uncorrelated with the X-ray emission. Not any point-like radio source is detected at the position of CXOU J174722.8-280915, the proposed neutron star. On the contrary, the X-ray source seems to lie within a small minimum in the radio emission.
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页码：365 / +
页数：2
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