3 citations · 4 across the 2 of their papers we have counts for
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Updated Pre-Main Sequence tracks at low metallicities for 0.1< M/Mo<1.5
Di Criscienzo, P. Ventura, F. D'Antona
Young populations at Z<Zo are being examined to understand the role of metallicity in the first phases of stellar evolution. For the analysis it is necessary to assign mass and age…
The self-enrichment scenario in intermediate metallicity globular clusters
Paolo Ventura, Francesca D'Antona
We present stellar yields computed from detailed models of intermediate mass asymptotic giant branch stars of low metallicity. In this work, the whole main microphysics inputs have…
The first stages of the evolution of Globular Clusters
Francesca D'Antona, Paolo Ventura, Vittoria Caloi
The majority of the inhomogeneities in the chemical composition of Globular Cluster (GC) stars appear due to primordial enrichment. The most studied model today claims that the eje…
Were most Low Mass X ray Binaries born in Globular Clusters?
Francesca D'Antona, Anamaria Teodorescu, Paolo Ventura
We summarize the status of art of the secular evolution of low mass X-ray binaries (LMXBs) and take a close look at the orbital period distribution of LMXBs and of binary milliseco…
Non-gray rotating stellar models and the evolutionary history of the Orion Nebular Cluster
Natália R. Landin, Paolo Ventura, Francesca D'Antona +2
Rotational evolution in the pre-main sequence (PMS) is described with new sets of PMS evolutionary tracks including rotation, non-gray boundary conditions (BCs) and either low (LCE…
Modelling the closest double degenerate system RXJ0806.3+1527 and its decreasing period
F. D'Antona, P. Ventura, L. Burderi +1
In the hypothesis that the 5.4m binary RXJ0806.3+1527 consists of a low mass helium white dwarf (donor) transferring mass towards its more massive white dwarf companion (primary),…