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Abundances of Be Stars in Very Young Open Clusters

Published online by Cambridge University Press:  12 April 2016

A. Marco ,
G. Bernabeu ,
J.M. Torrejón ,
J.J. Rodes  and
J. Fabregat
A. Marco
Affiliation:
Depariamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Ap.99, E-03080, Alicante, Spain
G. Bernabeu
Affiliation:
Depariamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Ap.99, E-03080, Alicante, Spain
J.M. Torrejón
Affiliation:
Depariamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Ap.99, E-03080, Alicante, Spain
J.J. Rodes
Affiliation:
Depariamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Ap.99, E-03080, Alicante, Spain
J. Fabregat
Affiliation:
Depariamento de Astronomía y Astrofísica, Universidad de Valencia, E-046100, Burjassot, Spain

Abstract

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We present here standard uvbyβ CCD photometry for five open clusters of the Galaxy in order to determine abundances of Be stars, as a function of age.

Type
1. Overview
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 59 - 62
Copyright
Copyright © Astronomical Society of the Pacific 2000

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