Millimeter-wave imaging of pulsar wind nebulae

被引：0
|
作者：
Bock, DCJ
Gaensler, BM
机构：
[1] Univ Calif Berkeley, Radio Astron Lab, Berkeley, CA 94720 USA
[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
来源：
YOUNG NEUTRON STARS AND THEIR ENVIRONMENTS | 2004年 / 218期
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We have observed the supernova remnants G16.7+0.1 and G29.7-0.3 at millimeter wavelengths with the Berkeley-Illinois-Maryland Association array, measuring total flux densities of the pulsar wind nebulae in the remnants. Our results imply a break at similar to 50 GHz in the spectrum of the PWN in C29.7-0.3, lower than previously estimated. The PWN in C16.7+0.1 either has a break < 100 GHz, or a steep radio spectrum.
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页码：207 / 210
页数：4
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