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researcher

J. Isern

86 papers hereh-index 517.6k citations344 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author2
  • first author17
  • middle author40
  • last author19

Across the 78 of 86 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR32
  • astro-ph31
  • astro-ph.HE10
  • astro-ph.GA6
  • hep-ph3
  • physics.ins-det2
same name
  • J. Isern — 36 papers, h 20
  • J. Isern — 4 papers
  • J. Isern — 4 papers, h 1
  • J. Isern — 2 papers, h 6
  • J. Isern — 1 paper, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

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
Showing 2013 · astro-ph.SRShow all

4 papers · 2 filters

astro-ph.SR2013★ 5 cited

White dwarf constraints on a varying G

Enrique García-Berro, Santiago Torres, Leandro G. Althaus +4

A secular variation of G modifies the structure and evolutionary time scales of white dwarfs. Using an state-of-the-art stellar evolutionary code, an up-to-date pulsational code,…

astro-ph.SR2013★ 37 cited

Detonations in white dwarf dynamical interactions

Gabriela Aznar-Siguán, Enrique García-Berro, Pablo Lorén-Aguilar +2

In old, dense stellar systems collisions of white dwarfs are a rather frequent phenomenon. Here we present the results of a comprehensive set of Smoothed Particle Hydrodynamics sim…

astro-ph.SR2013

Axion cooling of white dwarfs

J. Isern, S. Catalan, E. Garcia--Berro +2

The evolution of white dwarfs is a simple gravothermal process. This process can be tested in two ways, through the luminosity function of these stars and through the secular varia…

astro-ph.SR2013★ 25 cited

Magnetic white dwarfs with debris discs

Baybars Külebi, K. Yavuz Ekşi, Pablo Lorén-Aguilar +2

It has long been accepted that a possible mechanism for explaining the existence of magnetic white dwarfs is the merger of a binary white dwarf system, as there are viable mechanis…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.