Predicting low-frequency radio fluxes of known extrasolar planets

Free access article

Issue		A&A Volume 475, Number 1, November III 2007


Page(s)		359 - 368
Section		Planets and planetary systems
DOI		http://dx.doi.org/10.1051/0004-6361:20077397

A&A 475, 359-368 (2007)
DOI: 10.1051/0004-6361:20077397

Predicting low-frequency radio fluxes of known extrasolar planets

J.-M. Grießmeier¹, P. Zarka¹, and H. Spreeuw²

¹ LESIA, Observatoire de Paris, CNRS, UPMC, Université Paris Diderot; 5 Place Jules Janssen, 92190 Meudon, France
e-mail: [jean-mathias.griessmeier;philippe.zarka]@obspm.fr
² Astronomical Institute "Anton Pannekoek", Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
e-mail: hspreeuw@science.uva.nl

(Received 3 March 2007 / Accepted 18 August 2007 )

Abstract
Context. Close-in giant extrasolar planets ("Hot Jupiters") are believed to be strong emitters in the decametric radio range.
Aims.We present the expected characteristics of the low-frequency magnetospheric radio emission of all currently known extrasolar planets, including the maximum emission frequency and the expected radio flux. We also discuss the escape of exoplanetary radio emission from the vicinity of its source, which imposes additional constraints on detectability.
Methods.We compare the different predictions obtained with all four existing analytical models for all currently known exoplanets. We also take care to use realistic values for all input parameters.
Results. The four different models for planetary radio emission lead to very different results. The largest fluxes are found for the magnetic energy model, followed by the CME model and the kinetic energy model (for which our results are found to be much less optimistic than those of previous studies). The unipolar interaction model does not predict any observable emission for the present exoplanet census. We also give estimates for the planetary magnetic dipole moment of all currently known extrasolar planets, which will be useful for other studies.
Conclusions.Our results show that observations of exoplanetary radio emission are feasible, but that the number of promising targets is not very high. The catalog of targets will be particularly useful for current and future radio observation campaigns (e.g. with the VLA, GMRT, UTR-2 and with LOFAR).

Key words: radiation mechanisms: non-thermal -- catalogs -- plasmas -- planets and satellites general

What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.

If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.