Radio cyclotron emission from extra-solar planets

被引：0

作者：

Smith, Alexis ^{[1
]}

Cameron, Andrew ^{[1
]}

Greaves, Jane ^{[1
]}

Jardine, Moira ^{[1
]}

Langston, Glen ^{[2
]}

Backer, Donald ^{[3
]}

机构：

[1] Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9BX, Fife, Scotland

[2] Natl Radio Astron Observ, Green Bank, WV 24944 USA

[3] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

来源：

TRANSITING PLANETS, PROCEEDINGS | 2009年 / 253期

关键词：

D O I：

10.1017/S1743921308026926

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present results from an attempt to detect radio emission from the interaction between a transiting extra-solar planet and its host star. We determine a new upper limit of 47 mJy on the radio flux density from HD 189733b, in the frequency range 327-347 MHz.

引用

页码：456 / +

页数：2

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