1.7k citations · 2.8k across the 16 of their papers we have counts for
15 papers
The extended Main Sequence Turn Off cluster NGC1856: rotational evolution in a coeval stellar ensemble
F. D'Antona, M. Di Criscienzo, T. Decressin +3
Multiple or extended turnoffs in young clusters in the Magellanic Clouds have recently received large attention. A number of studies have shown that they may be interpreted as the…
Rapidly rotating second-generation progenitors for the blue hook stars of ω Cen
Marco Tailo, Francesca D'Antona, Enrico Vesperini +9
Horizontal Branch stars belong to an advanced stage in the evolution of the oldest stellar galactic population, occurring either as field halo stars or grouped in globular clusters…
Evolution of long-lived globular cluster stars I. Grid of stellar models with helium enhancement at [Fe/H] = -1.75
William Chantereau, Corinne Charbonnel, Thibaut Decressin
Our understanding of the formation and early evolution of globular clusters (GCs) has been totally overthrown with the discovery of the peculiar chemical properties of their long-l…
Pre-main sequence accretion and the formation of multiple populations in Globular Clusters
Francesca D'Antona, Paolo Ventura, Thibaut Decressin +2
We investigate the viability of a model in which the chemical anomalies among Globular Cluster stars are due to accretion of gas onto the protostellar discs of low mass stars. This…
Why the globular cluster NGC 6752 contains no sodium-rich second-generation AGB star
Corinne Charbonnel, William Chantereau, Thibaut Decressin +2
(Abridged) Globular clusters host multiple stellar populations showing different sodium enrichments. These various populations can be observed along the main sequence, red giant an…
Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002
Cyril Georgy, Sylvia Ekström, Patrick Eggenberger +11
(shortened) We provide a grid of single star models covering a mass range from 0.8 to 120 Msun with an initial metallicity Z = 0.002 with and without rotation. We discuss the impac…