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19992019
most citedIntermediate-mass star models with different helium and metal contents

163 citations · 869 across the 19 of their papers we have counts for

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9 papers · 1 filter

astro-ph2007★ 59 cited

The Peculiar Type Ib Supernova 2006jc: A WCO Wolf-Rayet Star Explosion

N. Tominaga, M. Limongi, T. Suzuki +21

We present a theoretical model for Type Ib supernova (SN) 2006jc. We calculate the evolution of the progenitor star, hydrodynamics and nucleosynthesis of the SN explosion, and the…

astro-ph2003★ 63 cited

Optical and near-infrared photometry of the Type Ia Supernova 2000E in NGC 6951

G. Valentini, E. Di Carlo, F. Massi +15

We present optical and near-infrared photometry, along with optical spectra, of the Type Ia supernova SN 2000E in the spiral galaxy NGC 6951. It was discovered by the staff of the…

astro-ph2002★ 100 cited

Carbon-Oxygen White Dwarfs Accreting CO-Rich Matter I: A Comparison Between Rotating and Non-Rotating Models

Luciano Piersanti, Simona Gagliardi, Icko Iben +1

We investigate the lifting effect of rotation on the thermal evolution of CO WDs accreting CO-rich matter. We find that rotation induces the cooling of the accreting star so that t…

astro-ph2002★ 63 cited

Optical and infrared observations of the supernova SN 1999el

E. Di Carlo, F. Massi, G. Valentini +22

Optical and near-infrared light curves of the Type IIn supernova 1999el in NGC 6951 are presented. A period of 220 days (416 days in the near-infrared) is covered from the first ob…

astro-ph2001★ 8 cited

The Influence of N14(e-,nu)C14(alpha,gamma)O18 reaction on the He-Ignition in Degenerate Physical Conditions

Luciano Piersanti, Santi Cassisi, Amedeo Tornambe'

The importance of NCO chain on the onset of the He-flash in degenerate physical conditions has been reevaluated. We find that low-mass, metal-rich (Z 0.001) structures climbi…

astro-ph2000★ 163 cited

Intermediate-mass star models with different helium and metal contents

G. Bono, F. Caputo, S. Cassisi +3

We present a comprehensive theoretical investigation of the evolutionary properties of intermediate-mass stars. The evolutionary sequences were computed from the Zero Age Main Sequ…