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Radio cyclotron emission from extra-solar planets
Published online by Cambridge University Press: 01 May 2008
Abstract
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S253: Transiting Planets , May 2008 , pp. 456 - 458
- Copyright
- Copyright © International Astronomical Union 2009