Non-Thermal Radio Emission from OB Stars: An Observer's View

被引：0
|
作者：
Benaglia, Paula [1 ]
机构：
[1] CCT La Plata CONICET, Inst Argentino Radioastron, La Plata, Buenos Aires, Argentina
来源：
HIGH ENERGY PHENOMENA IN MASSIVE STARS | 2010年 / 422卷
关键词：
MASS-LOSS; STELLAR WINDS; HOT STARS; SUBMILLIMETER OBSERVATIONS; CONTINUUM MEASUREMENTS; RADIATION; CATALOG; MULTIWAVELENGTH; BINARIES; SPECTRUM;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Some early-type stars are detectable radio emitters; their spectra can present both thermal and non-thermal contributions. Here I review the public radio data on OB stars, focusing on the non-thermal sources. The analysis of the statistical results gives rise to many open questions that are expected to be addressed, at least in part, with the upgrades of current radio telescopes and the upcoming new generation instruments.
引用
收藏
页码：111 / 121
页数：11
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