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Photographic magnitudes of 201 stars at 2600 Å

Published online by Cambridge University Press:  14 August 2015

Jean-Pierre Sivan
Affiliation:
Laboratoire d'Astronomie Spatiale du CNRS et Observatoire de Marseille, France
Maurice Viton
Affiliation:
Laboratoire d'Astronomie Spatiale du CNRS et Observatoire de Marseille, France

Abstract

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The magnitudes of 201 stars at 2600 Å (1000 Å passband) were derived from two plates of the winter Milky Way obtained with a large field camera. A preliminary investigation of the interstellar reddening allowed us to plot a color-spectral type diagram. Stars of type O seem to be brighter than predicted.

Résumé

Résumé

Les magnitudes de 201 étoiles à 2600 Å (longueur de la bande passante: 1000 Å) ont été obtenues grâce à deux photographies de la Voie Lactée d'hiver données par une caméra à grand champ. Une estimation préliminaire du rougissement interstellaire a permis de tracer un diagramme couleur-type spectral. Il semble que les étoiles O sont plus brillantes que prévu à 2600 Å.

Type
Part I: Stellar Fluxes
Copyright
Copyright © Reidel 1970 

References

Adams, T. F. and Morton, D. C.: 1968, Astrophys. J. 152, 195.CrossRefGoogle Scholar
Boggess, A. and Borgman, B.: 1964, Astrophys. J. 140, 1638.Google Scholar
Courtès, G.: Astronomie, Juin 1952.Google Scholar
Courtès, G.: 1960, Ann. Astrophys. 23, 115.Google Scholar
Hickok, F. R. and Morton, D. C.: 1968, Astrophys. J. 152, 203.CrossRefGoogle Scholar
Jaschek, M.: 1968, private communication.Google Scholar
Mihalas, D. M. and Morton, D. C.: 1965, Astrophys. J. 142, 253.CrossRefGoogle Scholar
Stecher, T. P.: 1965, Astrophys. J. 142, 1683.Google Scholar
Underhill, A. B.: 1963, Space Sci. Rev. 1, 749.CrossRefGoogle Scholar
Viton, M.: 1967, C. R. Acad. Sci. Paris 264, 1761.Google Scholar