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X-ray survey of the pleiades: dependence of X-ray luminosity on stellar age

Published online by Cambridge University Press:  04 August 2017

G. Micela ,
S. Sciortino ,
S. Serio ,
G.S. Vaiana ,
L. Golub ,
F.R. Harnden  and
R. Rosner
G. Micela
Affiliation:
Osservatorio Astronomico di Palermo
S. Sciortino
Affiliation:
Osservatorio Astronomico di Palermo
S. Serio
Affiliation:
Osservatorio Astronomico di Palermo Harvard-Smithsonian Center for Astrophysics
G.S. Vaiana
Affiliation:
Osservatorio Astronomico di Palermo Harvard-Smithsonian Center for Astrophysics
L. Golub
Affiliation:
Harvard-Smithsonian Center for Astrophysics
F.R. Harnden
Affiliation:
Harvard-Smithsonian Center for Astrophysics
R. Rosner
Affiliation:
Harvard-Smithsonian Center for Astrophysics

Extract

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The study of X-ray emission of stellar clusters, allows to decouple the influence of some individual stellar parameters, as initial conditions, composition and age, on the stellar X-ray luminosity function.

Type
I. EVOLUTION OF LOW AND INTERMEDIATE MASS STARS OBSERVATIONS AND MODELS
Information
Symposium - International Astronomical Union , Volume 105: Observational Tests of the Stellar Evolution Theory , 1984 , pp. 101 - 104
Copyright
Copyright © Reidel 1984 

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