Hostname: page-component-669899f699-ggqkh Total loading time: 0 Render date: 2025-05-03T20:16:42.839Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio Emissions from Terrestrial Planets around White Dwarfs

Published online by Cambridge University Press:  26 May 2016

Andrew Willes  and
Kinwah Wu
Andrew Willes
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
Kinwah Wu
Affiliation:
MSSL, University College London, RH5 6NT, United Kingdom

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Terrestrial planets in close orbits around magnetic white dwarf stars can be 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 the radio flux densities from white-dwarf/terrestrial-planet systems and discuss a scenario for the formation of these systems.

Type
Part 7: Cool Stars and their Planets
Information
Symposium - International Astronomical Union , Volume 219: Stars as Suns : Activity, Evolution and Planets , 2004 , pp. 390 - 394
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Bigg, E. K. 1964, Nature, 203, 1008.Google Scholar
Chanmugam, G. & Dulk, G. A. 1983, Annals of Israel Phys. Soc., 19, 223.Google Scholar
Clarke, J. T., et al. 2002, Nature, 415, 997.Google Scholar
Delamere, P. A., et al. 2003, J. Geophys. Res., 108, 1241.Google Scholar
Dulk, G. A. 1967, Icarus, 7, 173.Google Scholar
Goldreich, P. & Lynden-Bell, D. 1969, ApJ, 156, 59.CrossRefGoogle Scholar
Hakala, P., et al. 2003, MNRAS, 343, L10.Google Scholar
Hewitt, R. G., Melrose, D. B. & Rönnmark, K. G. 1981, PASA, 4, 221.CrossRefGoogle Scholar
Hill, T. W. & Vasyliunas, V. M. 2002, J. Geophys. Res., 107, 1464.Google Scholar
Kaiser, M. L., et al. 2000, J. Geophys. Res., 105, 16053.CrossRefGoogle Scholar
Li, J., Ferrario, L., & Wickramasinghe, D. T. 1998, ApJ, 503, L151.Google Scholar
Maeda, K. & Carr, T. D. 1992, J. Geophys. Res., 97, 1549.Google Scholar
Rybicki, K. R. & Denis, C. 2001, Icarus, 151, 130.CrossRefGoogle Scholar
Sackmann, I.-J., Boothroyd, A. I. & Kraemer, K. E. 1993, ApJ, 418, 457.Google Scholar
Soker, N. 2001, MNRAS, 324, 699.CrossRefGoogle Scholar
Strohmayer, T. E. 2002, ApJ, 581, 577.Google Scholar
Strohmayer, T. E. 2003, ApJ, 593, L39.CrossRefGoogle Scholar
Wickramasinghe, D. T. & Ferrario, L. 2000, PASP, 112, 873.Google Scholar
Willes, A. J. & Wu, K. 2003, MNRAS, submitted (astro-ph/0302583).Google Scholar
Wu, K., et al. 2002, MNRAS, 331, 221.Google Scholar