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Search for Rotational Modulation in Pre-Main Sequence Herbig Ae/Be Stars

Published online by Cambridge University Press:  19 July 2016

C. Catala
Affiliation:
Observatoire de Paris, Section de Meudon
J. Czarny
Affiliation:
Observatoire de Paris, Section de Meudon
P. Felenbok
Affiliation:
Observatoire de Paris, Section de Meudon

Extract

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The Herbig Ae/Be stars (Herbig, 1960; Finkenzeller and Hundt, 1984) are widely believed to be intermediate mass (2-5 M) pre-main sequence stars. In the past few years, a big effort has been made to model their outer layers, and it has been shown that they possess stellar winds and extended chromospheres (Catala et al., 1984; Catala et al., 1986a; Catala and Kunasz, 1987).

Type
II. Pre-Main-Sequence Stars
Copyright
Copyright © Kluwer 1988 

References

Références

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