Alvio Renzini
0000-0002-7093-7355
INAF-Osservatorio Astronomico di Padova
724 papers found
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Book-Review - Physical Processes in Red Giants
The role of semiconvection in bringing carbon to the surface of asymptotic giant branch stars of small core mass
Book-Review - Physical Processes in Red Giants - Proceedings - Erice Italy 1980SEP
Low mass Wolf-Rayet stars - Theory
The evolution of intermediate-mass stars
Carbon Stars in the Magellanic Clouds: Theory vs. Observations
Evolutionary Effects of Mass Loss in Low-Mass Stars
Advanced evolutionary stages of intermediate-mass stars. I. Evolution of surface compositions.
Red Giants as Precursors of Planetary Nebulae
The Globular Clusters in the Magellanic Clouds - Theoretical Considerations
Physical processes in red giants
Energetics of stellar populations
The variable stars in the Local Group of galaxies
On the origin of period changes in RR Lyrae stars.
Mass loss from red giants: some effects on the interstellar medium.
A new scenario for the formation of globular clusters and their peculiarities
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