Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..69...45a&link_type=abstract
Astrophysics and Space Science, vol. 69, no. 1, May 1980, p. 45-59.
Astronomy and Astrophysics
Astrophysics
18
Globular Clusters, Stellar Evolution, Stellar Models, Chemical Composition, Chronology, Dynamic Characteristics, Luminosity, Stellar Mass Ejection, Stellar Structure
Scientific paper
Synthetic and projected properties of models of globular clusters have been computed on the basis of stellar evolution and time changes of the dynamical cluster structure. Clusters with five and eight stellar groups (each group consisting of stars with the same mass) were studied. Mass loss from evolved stars was taken into account. Observational features were obtained at ages of 10 to 19 billion years. The basic importance of the horizontal- and asymptotic-branch stars is pointed out. A comparison of the results with observed data of M3 is discussed with the purpose of obtaining general indications rather than a specific fit.
Angeletti Lucio
Dolcetta R.
Giannone Pietro
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