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J/ApJ/612/511       Exoplanet radio emission                 (Lazio+, 2004)

The radiometric Bode's law and extrasolar planets. Lazio T.J.W., Farrell W.M., Dietrick J., Greenlees E., Hogan E., Jones C., Hennig L.A. <Astrophys. J., 612, 511-518 (2004)> =2004ApJ...612..511L
ADC_Keywords: Magnetic fields ; Radio sources ; Planets Keywords: magnetic fields - radio continuum: stars - solar wind Abstract: We predict the radio flux densities of the extrasolar planets in the current census, making use of an empirical relation - the radiometric Bode's law - determined from the five "magnetic" planets in the solar system (the Earth and the four gas giants). Radio emission from these planets results from solar wind-powered electron currents depositing energy in the magnetic polar regions. We find that most of the known extrasolar planets should emit in the frequency range 10-1000 MHz and, under favorable circumstances, have typical flux densities as large as 1mJy. We also describe an initial, systematic effort to search for radio emission in low radio frequency images acquired with the Very Large Array (VLA). The limits set by the VLA images (∼300mJy) are consistent with, but do not provide strong constraints on, the predictions of the model. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 45 113 Exoplanet radio emission
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 15 A15 --- Name Star name (1) 17- 20 F4.2 --- omega Planet's rotation rate relative to Jupiter's rate 22- 26 F5.2 [W] logP Log of the predicted power 28- 32 F5.1 --- mu The µ value (2) 34- 39 F6.1 MHz nu Frequency 41- 44 F4.1 [Jy] logS ? Log of the predicted burst flux density
Note (1): Planets are arranged roughly in order of increasing semi-major axis. Note (2): In units of Jupiter radii times the gravitational constant.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 23-Mar-2005
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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