Radio emissions from terrestrial planets around white dwarfs

Details Radio emissions from terrestrial planets around white dwarfs Radio emissions from terrestrial planets around white dwarfs

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26a...432.1091w&link_type=abstract

Astronomy and Astrophysics, Volume 432, Issue 3, March IV 2005, pp.1091-1100

Astronomy and Astrophysics

Astrophysics

15

Stars: Planetary Systems, Stars: White Dwarfs, Radiation Mechanisms: Non-Thermal, Radio Continuum: General

Scientific paper

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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