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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 ,
J. Czarny  and
P. Felenbok
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
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 105 - 108
Copyright
Copyright © Kluwer 1988 

References

Références

Catala, C., Kunasz, P., Praderie, F.: 1984, Astron. Astrophys. 134, 402 Google Scholar
Catala, C., Czarny, J., Felenbok, P., Praderie, F.: 1986a, Astron. Astrophys. 154, 103 Google Scholar
Catala, C., Felenbok, P., Czarny, J., Talavera, A., Boesgaard, A.M.: 1986b, Astrophys. J. 308, 791 CrossRefGoogle Scholar
Catala, C., Kunasz, P.B.: 1987, Astron. Astrophys. 174, 158 Google Scholar
Finkenzeller, U., Mundt, R.: 1984, Astron. Astrophys. Suppl. 55, 109 Google Scholar
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Praderie, F., Simon, T., Catala, C., Boesgaard, A.M.: 1986, Astrophys. J. 303, 311.CrossRefGoogle Scholar