Candidates for detecting exoplanetary radio emissions generated by magnetosphere–ionosphere coupling
Article first published online: 9 OCT 2012
© 2012 The Author Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society: Letters
Volume 427, Issue 1, pages L75–L79, November 2012
How to Cite
Nichols, J. D. (2012), Candidates for detecting exoplanetary radio emissions generated by magnetosphere–ionosphere coupling. Monthly Notices of the Royal Astronomical Society: Letters, 427: L75–L79. doi: 10.1111/j.1745-3933.2012.01348.x
- Issue published online: 7 NOV 2012
- Article first published online: 9 OCT 2012
- Accepted 2012 September 4. Received 2012 September 4; in original form 2012 June 8
Relations. Proxies for LX.
Figure. Radio powers versus orbital distance.
Table 1. The potential targets for observing internally generated exoplanetary radio emissions amongst stars known already to host planets.
Table 2. As for Table 1, but for any star with LX > 100 LX⊙.
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