Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-12T08:33:06.347Z Has data issue: false hasContentIssue false

Radio Evidence for Nonthermal Particle Acceleration in Normal Stars

Published online by Cambridge University Press:  25 May 2016

K. R. Lang*
Affiliation:
Department of Physics and Astronomy, Tufts University, Medford, MA 02155, U.S.A.

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.

The Very Large Array has been used to detect nonthermal radio emission from nearby stars of late spectral type F, G, K, and M, and has provided unique high-resolution investigations of the Sun's radio emission.

Type
Part I: Talks
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Güdel, M., & Benz, A. O. 1993, ApJ, 405, L63.CrossRefGoogle Scholar
Hempelmann, A., Schmitt, J. H. M. M., Schultz, M., Ruediger, G., & Stepien, K. 1995, A&A, 294, 515.Google Scholar
Krucker, S., & Benz, A. O. 1998, ApJ, 501, L213.CrossRefGoogle Scholar
Lang, K. R. 1994, ApJS, 90, 753.Google Scholar
Lang, K. R. 1995, Sun, Earth and Sky (New York: Springer-Verlag).Google Scholar
Lang, K. R. 1996, in Magnetohydrodynamic Phenomena in the Solar System, eds. Uchida, Y. et al. (Boston: Kluwer).Google Scholar
Lang, K. R. 1999, Surveys in Geophysics, 19, 521.CrossRefGoogle Scholar
Pallavicini, R., Golub, L., Rosner, R., Vaiana, G. S., Ayres, T., & Linsky, J. L. 1981, ApJ, 248, 279.Google Scholar
Willson, R. F., Redfield, S. L., Lang, K. R., Thompson, B. J., & St. Cyr, O. C. 1998, ApJ, 504, L117.Google Scholar