Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S253(4), p. 456-458, 2008

DOI: 10.1017/s1743921308026926

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Radio cyclotron emission from extra-solar planets

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

AbstractWe 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.

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