activity
19972022
most citedEvolutionary and pulsational properties of white dwarf stars

405 citations · 5.5k across the 84 of their papers we have counts for

collaborators

86 papers

astro-ph.SR2022★ 18 cited

Can we reveal the core-chemical composition of ultra-massive white dwarfs through their magnetic fields?

Maria E. Camisassa, Roberto Raddi, Leandro G. Althaus +5

Ultra-massive white dwarfs () are particularly interesting objects that allow us to study extreme astrophysical phenomena such as type Ia superno…

astro-ph.HE2022★ 29 cited

Observations of the Very Young Type Ia Supernova 2019np with Early-excess Emission

Hanna Sai, Xiaofeng Wang, Nancy Elias-Rosa +30

Early-time radiative signals from type Ia supernovae (SNe Ia) can provide important constraints on the explosion mechanism and the progenitor system. We present observations and an…

astro-ph.HE2022

Search for gamma-ray emission from a galactic supernova with the anticoincidence system of SPI

Mariona Caixach, Pierre Jean, Jordi Isern +1

The detection of the very early gamma-emission of a Type Ia supernova (SNIa) could provide a deep insight on the explosion mechanism and nature of the progenitor. However this has…

astro-ph.HE2021

EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade

R. Alves Batista, M. A. Amin, G. Barenboim +134

Astroparticle physics is undergoing a profound transformation, due to a series of extraordinary new results, such as the discovery of high-energy cosmic neutrinos with IceCube, the…

astro-ph.HE2021★ 4 cited

Synthesis of radioactive elements in novae and supernovae and their use as a diagnostic tool

J. Isern, M. Hernanz, E. Bravo +5

Novae and supernovae play a key role in many fields of Astrophysics and Cosmology. Despite their importance, an accurate description of which objects explode and why and how they e…

astro-ph.SR2020★ 4 cited

White Dwarfs as Advanced Physics Laboratories. The Axion case

Jordi Isern

The shape of the luminosity function of white dwarfs (WDLF) is sensitive to the characteristic cooling time and, therefore, it can be used to test the existence of additional sourc…