Skip to main content Accessibility help

Radio cyclotron emission from extra-solar planets

  • Alexis Smith (a1), Andrew Cameron (a1), Jane Greaves (a1), Moira Jardine (a1), Glen Langston (a2) and Donald Backer (a3)...


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.


Corresponding author


Hide All
Collier Cameron, A. et al. 2006, MNRAS, 373, 799
Grießmeier, J. M., Motschmann, U., Glassmeier, K. H., Mann, G., & Rucker, H. O. 2006, in Arnold, L., Bouchy, F. & Moutou, C. (eds.), Tenth anniversary of 51 Peg-b: Status of and prospects for hot Jupiter studies., Colloquium held at Observatoire de Haute Provence, France, August 22-25, 2005. (Frontier Group, Paris), p. 259
Jardine, M. & Cameron, A. et al. , in preparation.
Lazio, T., Joseph, W., Farrell, W.M., Dietrick, J., Greenless, E., Hogan, E., Jones, C., & Hennig, L. A. 2004, ApJ, 612, 511
Moutou, C., Donati, J.-F., Savalle, R., Hussain, G., Alecian, E., Bouchy, F., Catala, C., Collier Cameron, A., Udry, S., & Vidal-Madjar, A. 2007, A&A, 473, 651
MathJax is a JavaScript display engine for mathematics. For more information see


Full text views

Total number of HTML views: 0
Total number of PDF views: 0 *
Loading metrics...

Abstract views

Total abstract views: 0 *
Loading metrics...

* Views captured on Cambridge Core between <date>. This data will be updated every 24 hours.

Usage data cannot currently be displayed