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Statistical analysis of the red giant distributions of old open clusters

Published online by Cambridge University Press:  04 August 2017

G. Barbaro  and
L. Pigatto
G. Barbaro
Affiliation:
Istituto di Astronomia, Università di Padova, Osservatorio Astronomico, Padova
L. Pigatto
Affiliation:
Istituto di Astronomia, Università di Padova, Osservatorio Astronomico, Padova

Extract

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In order to verify the agreement with the theory of the observed HR diagram as a whole, 38 open clusters with (B-V)o, t≥0.10 at the turnoff, have been analyzed with particular regard to the RGB luminosity function.

Type
I. EVOLUTION OF LOW AND INTERMEDIATE MASS STARS OBSERVATIONS AND MODELS
Information
Symposium - International Astronomical Union , Volume 105: Observational Tests of the Stellar Evolution Theory , 1984 , pp. 97 - 100
Copyright
Copyright © Reidel 1984 

References

Bertelli, G., Bressan, A.: private communication.Google Scholar
Ciardullo, R.B., Demarque, P.: 1977, Yale Trans., Vol. 33.Google Scholar
Ciardullo, R.B., Demarque, P.: 1979, Dud. Obs. Rpt. 14, 317.Google Scholar
Johnson, H.L.: 1966, Ann. Rev. Astron. Astrophys. 4, 193.CrossRefGoogle Scholar
Lee, T.A.: 1970, Astrophys. J. 162, 217.Google Scholar
Maeder, A.: 1975, Astron. Astrophys. 43, 61.Google Scholar
Maeder, A.: 1976, Astron. Astrophys. 47, 389.Google Scholar
Morton, D.C.: 1969, Astrophys. J. 158, 629.Google Scholar
Morton, D.C., Adams, T.F.: 1968, Astrophys. J. 151, 611.Google Scholar
Sweigart, A.V., Gross, P.G.: 1976, Astrophys. J. Suppl. 32, 367.Google Scholar