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Fundamental Parameters : Normal A0 Dwarf Stars of the Solar Neighbourhood

Published online by Cambridge University Press:  14 August 2015

M. Gerbaldi ,
R. Faraggiana ,
R. Burnage ,
F. Delmas ,
A. Gomez  and
S. Grenier
M. Gerbaldi
Affiliation:
CNRS and Université de Paris Sud XI Institut d’Astrophysique98bis, Bd. Arago, 75014 Paris, France
R. Faraggiana
Affiliation:
Dipartimento di Astronomia v. Tiepolo 11, 34131 TriesteItaly
R. Burnage
Affiliation:
CNRS, Observatoire de Haute Provence04870 Saint Michel l’Observatoire, France
F. Delmas
Affiliation:
CNRS Institut d’Astrophysique98bis, Bd. Arago, 75014 Paris, France
A. Gomez
Affiliation:
DASGAL, Observatoire de Meudon, 92150 Meudon, France
S. Grenier
Affiliation:
DASGAL, Observatoire de Meudon, 92150 Meudon, France

Extract

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The purpose of this paper is to define a set of “standard”, “reference” or “comparison” stars, according to their use, of spectral type A0V in order to be used for further studies in the domain of peculiar stars as well as normal stars of this Teff and luminosity range.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 11 , Issue 2: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part B), 1997 , 1998 , pp. 653 - 656
Copyright
Copyright © Kluwer 1998

References

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