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Gabriela Aznar–Siguán

3 papers here

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

author position
  • first author1
  • last author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
ORCID 0000-0002-1947-4703

identity via Semantic Scholar / OpenAlex

most citedSpiral Disk Instability Can Drive Thermonuclear Explosions in Binary White Dwarf Mergers

46 citations · 105 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2015★ 46 cited

Spiral Disk Instability Can Drive Thermonuclear Explosions in Binary White Dwarf Mergers

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

Thermonuclear, or Type Ia supernovae (SNe Ia), originate from the explosion of carbon--oxygen white dwarfs, and serve as standardizable cosmological candles. However, despite their…

astro-ph.SR2014★ 39 cited

The response of a helium white dwarf to an exploding type Ia supernova

Oded Papish, Noam Soker, Enrique García-Berro +1

We conduct numerical simulations of the interacting ejecta from an exploding CO white dwarf (WD) with a He WD donor in the double-detonation scenario for Type Ia supernovae (SNe Ia…

astro-ph.SR2014★ 20 cited

On the possible observational signatures of white dwarf dynamical interactions

G. Aznar-Siguán, E. García-Berro, M. Magnien +1

We compute the possible observational signatures of white dwarf dynamical interactions in dense stellar environments. Specifically, we compute the emission of gravitational waves,…

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