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Comment on photometric evolutionary corrections

Published online by Cambridge University Press:  12 April 2016

John P. Huchra
John P. Huchra*
Affiliation:
Hale Observatories, California Institute of Technology, Carnegie Institution of Washington

Extract

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De récentes études de galaxies très bleues montrent que la formation des étoiles a lieu avec une fonction initiale de masse plus riche en étoiles de masse élevée que la fonction de Salpeter.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 37: Décalages vers le rouge et Expansion de l’Univers , 1977 , pp. 179 - 181
Copyright
Copyright © Editions du CNRS 1977

References

Huchra, J. P. 1976, Ph.D. Thesis, California Institute of Technology.Google Scholar
Salpeter, E. 1955, Ap. J., 121, 161.Google Scholar
Sandage, A., and Tammann, , 1974, Ap. J., 191, 603.Google Scholar
Searle, L., Sargent, W. L. W., and Bagnuolo, W. 1973, Ap. J., 179, 427.Google Scholar
Tinsley, B. 1968, Ap. J., 151, 547.Google Scholar
Tinsley, B. 1972a, Astr. and Ap., 20, 383.Google Scholar
Tinsley, B. 1972b, Ap. J. (Letters), 173, L97.CrossRefGoogle Scholar
Tinsley, B., and Gunn, J. E. 1976, Ap. J., 203, 52.Google Scholar