activity
19972022
most citedEvolutionary and pulsational properties of white dwarf stars

405 citations · 4.9k across the 99 of their papers we have counts for

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Showing 2012Show all

8 papers · 1 filter

astro-ph.GA2012★ 12 cited

White dwarf cooling sequences and cosmochronology

J. Isern, A. Artigas, E. Garcia-Berro

The evolution of white dwarfs is a simple gravothermal process. This means that their luminosity function, i.e. the number of white dwarfs per unit bolometric magnitude and unit vo…

astro-ph.SR2012★ 1 cited

The impact of mergers in the mass distribution of white dwarfs

J. Isern, S. Catalan, E. Garcia-Berro +1

Recent surveys have allowed to derive the white dwarf mass distribution with reasonable accuracy. This distribution shows a noticeable degree of structure that it is often attribut…

astro-ph.SR2012

On the origin of high-field magnetic white dwarfs

E. García-Berro, S. Torres, P. Lorén-Aguilar +6

High-field magnetic white dwarfs have been long suspected to be the result of stellar mergers. However, the nature of the coalescing stars and the precise mechanism that produces t…

astro-ph.SR2012★ 50 cited

Outer boundary conditions for evolving cool white dwarfs

R. D. Rohrmann, L. G. Althaus, E. García-Berro +2

White dwarf evolution is essentially a gravothermal cooling process, which,for cool white dwarfs, sensitively depends on the treatment of the outer boundary conditions. We provide…

astro-ph.IM2012★ 1 cited

The on-board data handling concept for the LOFT Large Area Detector

S. Suchy, P. Uter, C. Tenzer +9

The Large Observatory for X-ray Timing (LOFT) is one of the four candidate ESA M3 missions considered for launch in the time-frame of 2022. It is specifically designed to perform f…

astro-ph.SR2012★ 88 cited

Explaining the type Ia supernova PTF 11kx with a violent-prompt merger scenario

Noam Soker, Amit Kashi, Enrique Garcia-Berro +2

We argue that the multiple shells of circumstellar material (CSM) and the supernovae (SN) ejecta interaction with the CSM starting 59 days after the explosion of the Type Ia SN (SN…