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F. Schneider

4 papers hereh-index 685 citations12 works total

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

author position
  • middle author3
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.HE1
same name
  • F. Schneider — 12 papers, h 8
  • F. Schneider — 11 papers, h 10
  • F. Schneider — 3 papers, h 3
  • F. Schneider — 1 paper, h 1
  • F. Schneider — 1 paper, h 27
  • F. Schneider — 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

collaborators

4 papers

astro-ph.HE2025

NLTE spectral modelling for a carbon-oxygen and helium white-dwarf merger as a Ca-rich transient candidate

F. P. Callan, A. Holas, J. Morán-Fraile +7

We carry out NLTE (non local thermodynamic equilibrium) radiative transfer simulations to determine whether explosion during the merger of a carbon-oxygen (CO) white dwarf (WD) wit…

astro-ph.SR2025

Magnetically driven outflows in 3D common-envelope evolution of massive stars

Marco Vetter, Friedrich K. Roepke, Fabian R. N. Schneider +7

Recent three-dimensional magnetohydrodynamical simulations of the common-envelope interaction revealed the self-consistent formation of bipolar magnetically driven outflows launche…

astro-ph.SR2024

From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral

M. Vetter, F. K. Roepke, F. R. N. Schneider +4

Three-dimensional simulations usually fail to cover the entire dynamical common-envelope phase of gravitational wave progenitor systems due to the vast range of spatial and tempora…

astro-ph.SR2024

Large-scale ordered magnetic fields generated in mergers of helium white dwarfs

Rüdiger Pakmor, Ingrid Pelisoli, Stephen Justham +9

Stellar mergers are one important path to highly magnetised stars. Mergers of two low-mass white dwarfs may create up to every third hot subdwarf star. The merging process is usual…

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