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most citedSuper and massive AGB stars - IV. Final fates - Initial to final mass relation

261 citations · 1.2k across the 21 of their papers we have counts for

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astro-ph2006★ 40 cited

The late stages of the evolution of intermediate-mass primordial stars: the effects of overshooting

Pilar Gil-Pons, Jordi Gutierrez, Enrique Garcia-Berro

We compute and analyze the evolution of primordial stars of masses at the ZAMS between 5 M_sun and 10 M_sun, with and without overshooting. Our main goals are to determine the natu…

astro-ph2005★ 40 cited

The formation of DA white dwarfs with thin hydrogen envelopes

L. G. Althaus, M. M. Miller Bertolami, A. H. Córsico +2

We study the formation and evolution of DA white dwarfs, the progenitors of which have experienced a late thermal pulse (LTP) shortly after the departure from the thermally pulsing…

astro-ph2004★ 27 cited

Carbon burning in intermediate mass primordial stars

P. Gil-Pons, T. Suda, M. Y. Fujimoto +1

The evolution of a zero metallicity 9 M_s star is computed, analyzed and compared with that of a solar metallicity star of identical ZAMS mass. Our computations range from the main…

astro-ph2003★ 17 cited

The Impact of the Chemical Stratification of White Dwarfs on the Classification of Classical Novae

Jordi Jose, Margarita Hernanz, Enrique Garcia-Berro +2

We analyse the impact of the initial abundances of the underlying white dwarf core on the nucleosynthesis accompanying classical nova outbursts, in the framework of hydrodynamic mo…

astro-ph2003★ 51 cited

The frequency of occurrence of novae hosting an ONe white dwarf

P. Gil-Pons, E. Garcia-Berro, J. Jose +2

In this paper, we revisit the problem of the determination of the frequency of occurrence of galactic nova outbursts which involve an oxygen-neon (ONe) white dwarf. The improvement…

astro-ph2002★ 14 cited

On the formation of Super-AGB stars in intemediate mass close binary systems

Pilar Gil-Pons, Enrique Garcia-Berro

The evolution of a star of initial mass 9 M_s, and Z = 0.02 in a Close Binary System is followed in the presence of different mass companions in order to study their influence on t…