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Thermally Pulsing AGB Models of Intermediate Mass Stars
O. Straniero, M. Limongi, A. Chieffi +3
We present a set of models of AGB stars with initial mass larger than 5 Mo as obtained with the FRANEC code. It includes models of Z=0.02 and Z=0.001, with and without mass loss.
Do zero metal intermediate mass stars experience thermal pulses?
I. Dominguez, O. Straniero, M. Limongi +1
We have studied the evolution of intermediate mass (M.ge.5Mo) zero metal (Z=0) stars with particular attention to the AGB phase. At variance with previous claims we find that these…
The Large Magellanic Cloud globular cluster NGC 1866: new data, new models, new analysis
Vincenzo Testa, Francesco R. Ferraro, Alessandro Chieffi +3
We present a new deep (down to V ~ 24) photometry of a wide region (6'x 6') around the LMC globular cluster NGC1866: our sample is complete, down to 3 mag below the brightest MS st…
The giant, horizontal and asymptotic branches of galactic globular clusters. I. The catalog, photometric observables and features
F. R. Ferraro, M. Messineo, F. Fusi Pecci +4
A catalog including a set of the most recent Color Magnitude Diagrams (CMDs) is presented for a sample of 61 Galactic Globular Clusters (GGCs). We used this data-base to perform an…
Intermediate mass stars: updated models
Inma Dominguez, Alessandro Chieffi, Marco Limongi +1
A new set of stellar models in the mass range 1.2 to 9 is presented. The adopted chemical compositions cover the typical galactic values, namely …
The Luminosity Function of M3
R. T. Rood, E. Carretta, B. Paltrinieri +6
We present a high precision, large sample luminosity function (LF) for the Galactic globular cluster M3. With a combination of ground based and Hubble Space Telescope data we cover…