Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S253(4), p. 456-458, 2008
DOI: 10.1017/s1743921308026926
Full text: Unavailable
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.