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The luminosity function of the SMC clusters NGC152 and K3

Published online by Cambridge University Press:  04 August 2017

M. Kontizas ,
E. Kontizas  and
N. Stewart
M. Kontizas
Affiliation:
University of Athens, Observatory of Athens, University of Edinburgh
E. Kontizas
Affiliation:
University of Athens, Observatory of Athens, University of Edinburgh
N. Stewart
Affiliation:
University of Athens, Observatory of Athens, University of Edinburgh

Extract

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In a previous investigation of the Luminosity Functions (LF) it was found that some SMC clusters show significant characteristics like the very large number of stars at Mv = O. Omag and a gap just below the Horizontal Branch (HB) like feature of their colour-magnitude (c-m) diagram (Kontizas and Kontizas, 1982).

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. 121 - 122
Copyright
Copyright © Reidel 1984 

References

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