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Energy Distributions of Be Stars: (Review Paper)

Published online by Cambridge University Press:  14 August 2015

R. E. Schild
R. E. Schild*
Affiliation:
Center for Astrophysics, Harvard College Observatory and Smithsonian Astrophysical Observatory, Cambridge, Mass., U.S.A.

Abstract

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Energy distributions from 0.32 to 1.06 μ for field Be stars having p designations in their spectral types show that stars with Balmer discontinuities in emission do exist. Furthermore, the filling in of the Balmer continuum near the discontinuity is usually observed. The continuum emission showing a peak near 1 μ is a common feature in the energy distributions presented here.

Energy distributions for a number of bright field Be stars are also presented and discussed.

Type
Part 1: Observations of Be Stars
Information
Symposium - International Astronomical Union , Volume 70: Be and Shell Stars , 1976 , pp. 107 - 119
Copyright
Copyright © Reidel 1976 

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