activity
20152022
most citedWhite dwarf evolutionary sequences for low-metallicity progenitors: The impact of third dredge-up

107 citations · 428 across the 9 of their papers we have counts for

collaborators

15 papers

astro-ph.SR202263 cited

Spectral classification of the 100 pc white dwarf population from Gaia-DR3 and the Virtual Observatory

F. M. Jiménez-Esteban, S. Torres, A. Rebassa-Mansergas +5

The third data release of Gaia has provided low resolution spectra for ~100,000 white dwarfs (WDs) that, together with the excellent photometry and astrometry, represent an unrival…

astro-ph.SR202227 cited

The evolution of ultra-massive carbon oxygen white dwarfs

María E. Camisassa, Leandro G. Althaus, Detlev Koester +3

Ultra-massive white dwarfs () are considered powerful tools to study type Ia supernovae explosions, merger events, the occurrence of physical p…

astro-ph.SR202140 cited

Constraining the solar neighbourhood age-metallicity relation from white dwarf-main sequence binaries

A. Rebassa-Mansergas, J. Maldonado, R. Raddi +11

The age-metallicity relation is a fundamental tool for constraining the chemical evolution of the Galactic disc. In this work we analyse the observational properties of this relati…

astro-ph.GA202137 cited

The Gaia DR2 halo white dwarf population: the luminosity function, mass distribution and its star formation history

Santiago Torres, Alberto Rebassa-Mansergas, María E. Camisassa +1

We analyze the volume-limited nearly complete 100 pc sample of 95 halo white dwarf candidates identified by the second data release of Gaia. Based on a detailed population synthesi…

astro-ph.SR202049 cited

The formation of ultra-massive carbon-oxygen core white dwarfs and their evolutionary and pulsational properties

Leandro G. Althaus, Pilar Gil Pons, Alejandro H. Córsico +6

(Abridged abstract) We explore the formation of ultra-massive (M_{\rm WD} \gtrsim 1.05 M_\sun$), carbon-oxygen core white dwarfs resulting from single stellar evolution. We also st…

astro-ph.SR202060 cited

An ultra-massive white dwarf with a mixed hydrogen-carbon atmosphere as a likely merger remnant

Mark A. Hollands, Pier-Emmanuel Tremblay, Boris T. Gänsicke +11

White dwarfs are dense, cooling stellar embers consisting mostly of carbon and oxygen, or oxygen and neon (with a few percent carbon) at higher initial stellar masses. These stella…