期刊
ASTRONOMY & ASTROPHYSICS
卷 432, 期 3, 页码 1091-1100出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20040417
关键词
stars : planetary systems; stars : white dwarfs; radiation mechanisms : non-thermal; radio continuum : general
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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