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The Structure and Energy Balance in Main Sequence Stars

Published online by Cambridge University Press:  12 April 2016

C. Jordan ,
T.R. Ayres  and
A. Brown
C. Jordan
Affiliation:
Department of Theoretical Physics, Oxford University, UK
T.R. Ayres
Affiliation:
LASP, University of Colorado, Boulder, USA
A. Brown
Affiliation:
Department of Physics, Queen Mary College, London, UK

Abstract

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High-resolution spectra obtained with the IUE satellite have been used to study the structure and energy balance in the main sequence stars ξ Boo A, α Cen A, α Cen B and ε Eri. The EUV observations are combined with X-ray fluxes to predict the coronal temperatures, the electron pressures and energy lost or transferred by radiation and thermal conduction

Type
Session I: General Characteristics of Active Dwarfs
Information
International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 61 - 65
Copyright
Copyright © Reidel 1983

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