activity
20052019
most citedNew cooling sequences for old white dwarfs

252 citations · 2.5k across the 57 of their papers we have counts for

collaborators

57 papers

astro-ph.SR2019★ 16 cited

The effects of Ne sedimentation and metallicity on the local 40 pc white dwarf luminosity function

Jordi Tononi, Santiago Torres, Enrique García-Berro +3

We analyze the effect of the sedimentation of Ne on the local white dwarf luminosity function by studying scenarios under different Galactic metallicity models. We make use…

astro-ph.SR2018★ 134 cited

On the evolution of ultra-massive white dwarfs

María E. Camisassa, Leandro G. Althaus, Alejandro H. Córsico +6

Ultra-massive white dwarfs are powerful tools to study various physical processes in the Asymptotic Giant Branch (AGB), type Ia supernova explosions and the theory of crystallizati…

astro-ph.CO2018★ 5 cited

Spatial variation of fundamental constants: testing models with thermonuclear supernovae

Carolina Negrelli, Lucila Kraiselburd, Susana J. Landau +1

Since Dirac stated his Large Number Hypothesis the space-time variation of fundamental constants has been an active subject of research. Here we analyze the possible spatial variat…

astro-ph.GA2018★ 5 cited

The population of single and binary white dwarfs of the Galactic bulge

S. Torres, E. García-Berro, R. Cojocaru +1

Recent Hubble Space Telescope observations have unveiled the white dwarf cooling sequence of the Galactic bulge. Although the degenerate sequence can be well fitted employing the m…

astro-ph.SR2017★ 16 cited

One-Armed Spiral Instability in Double-Degenerate Post-Merger Accretion Disks

Rahul Kashyap, Robert Fisher, Enrique García-Berro +3

Increasing observational and theoretical evidence points to binary white dwarf mergers as the origin of some if not most normal Type Ia supernovae (SNe Ia). In this paper, we discu…

astro-ph.HE2017★ 10 cited

White dwarf dynamical interactions and fast optical transients

Enrique García-Berro, Carles Badenes, Gabriela Aznar-Siguán +1

Recent advances in time-domain astronomy have uncovered a new class of optical transients with timescales shorter than typical supernovae and a wide range of peak luminosities. Sev…