4.6 Article

Radio emissions from terrestrial planets around white dwarfs

Journal

ASTRONOMY & ASTROPHYSICS
Volume 432, Issue 3, Pages 1091-1100

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361:20040417

Keywords

stars : planetary systems; stars : white dwarfs; radiation mechanisms : non-thermal; radio continuum : general

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Terrestrial planets in close orbits around magnetic white dwarf stars are potential electron-cyclotron maser sources, by analogy to planetary radio emissions generated from the electrodynamic interaction between Jupiter and the Galilean moons. We present predictions of radio flux densities and the number of detectable white-dwarf/terrestrial-planet systems, and discuss a scenario for their formation.

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