most citedEvolution of white dwarf stars with high-metallicity progenitors: the role of 22Ne diffusion

68 citations · 85 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2011★ 17 cited

The white dwarf cooling sequence of NGC 6791: a unique tool for stellar evolution

E. García-Berro, S. Torres, I. Renedo +5

NGC 6791 is a well-studied, metal-rich open cluster that is so close to us that can be imaged down to luminosities fainter than that of the termination of its white dwarf cooling s…

astro-ph.SR2010★ 68 cited

Evolution of white dwarf stars with high-metallicity progenitors: the role of 22Ne diffusion

Leandro G. Althaus, Enrique García-Berro, Isabel Renedo +3

Motivated by the strong discrepancy between the main sequence turn-off age and the white dwarf cooling age in the metal-rich open cluster NGC 6791, we compute a grid of white dwarf…

astro-ph.SR2010

New chemical profiles for the asteroseismology of ZZ Ceti stars

L. G. Althaus, A. H. Córsico, A. Bischoff-Kim +4

We compute new chemical profiles for the core and envelope of white dwarfs appropriate for pulsational studies of ZZ Ceti stars. These profiles are extracted from the complete evol…

astro-ph.SR2010

A white dwarf cooling age of 8 Gyr for NGC 6791 from physical separation processes

Enrique García-Berro, Santiago Torres, Leandro G. Althaus +6

NGC 6791 is a well studied open cluster1 that it is so close to us that can be imaged down to very faint luminosities. The main sequence turn-off age (~8 Gyr) and the age derived f…

astro-ph.SR2010

New cooling sequences for old white dwarfs

Isabel Renedo, Leandro G. Althaus, Marcelo M. Miller Bertolami +4

We present full evolutionary calculations appropriate for the study of hydrogen-rich DA white dwarfs. This is done by evolving white dwarf progenitors from the zero age main sequen…