27 citations · 51 across the 3 of their papers we have counts for
3 papers
astro-ph.SR2022★ 2 cited
White-dwarf asteroseismology with the {\sl TESS} space telescope
A. H. Córsico
As white-dwarf (WD) stars cool, they go through one or more stages of (gravity)-mode pulsational instability, becoming multiperiodic variable stars. Stars passing through these…
astro-ph.SR2022★ 27 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.SR2022★ 22 cited
An evolutionary channel for CO-rich and pulsating He-rich subdwarfs
Marcelo M. Miller Bertolami, Tiara Battich, Alejandro H. Córsico +2
Recently a new class of hot subluminous stars strongly enriched in C and O have been discovered (CO-sdOs). These stars show abundances very similar to those observed in PG1159 star…