Willes, AJ;
Wu, K;
(2005)
Radio emissions from terrestrial planets around white dwarfs.
ASTRON ASTROPHYS
, 432
(3)
1091 - 1100.
10.1051/0004-6361:20040417.
![[thumbnail of 10199.pdf]](https://discovery-pp.ucl.ac.uk/style/images/fileicons/application_pdf.png) Preview |
PDF
10199.pdf Download (391kB) |
Abstract
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.
| Type: | Article |
|---|---|
| Title: | Radio emissions from terrestrial planets around white dwarfs |
| Open access status: | An open access version is available from UCL Discovery |
| DOI: | 10.1051/0004-6361:20040417 |
| Keywords: | stars : planetary systems, stars : white dwarfs, radiation mechanisms : non-thermal, radio continuum : general, LOW-MASS STARS, EXTRASOLAR PLANETS, PERIOD BINARY, GIANT, IO, SOLAR, LUMINOSITY, MAGNETISM, ROTATION, GANYMEDE |
| UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics |
| URI: | https://discovery-pp.ucl.ac.uk/id/eprint/10199 |
Archive Staff Only
 |
View Item |
