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researcher

F. Schneider

5 papers here

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

author position
  • first author1
  • middle author2

Across the 3 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR5
same name
  • F. Schneider — 23 papers, h 27
  • F. Schneider — 3 papers, h 10
  • F. Schneider — 2 papers
  • F. Schneider — 1 paper, h 1
  • F. Schneider — 1 paper, h 35
  • F. Schneider — 1 paper, h 16

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
20192023
most citedLong-term evolution of a magnetic massive merger product

76 citations · 153 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2023★ 1 cited

Contact tracing of binary stars: Pathways to stellar mergers

Jan Henneco, Fabian R. N. Schneider, Eva Laplace

Stellar mergers lead to diverse phenomena: rejuvenated blue stragglers, magnetised and peculiar stars, transients and nebulae. Using a grid of about 6000 detailed 1D binary evoluti…

astro-ph.SR2020

Pre-supernova evolution, compact object masses and explosion properties of stripped binary stars

F. R. N. Schneider, Ph. Podsiadlowski, B. Müller

Most massive stars are born in binary or higher-order multiple systems and exchange mass with a companion during their lives. In particular, the progenitors of a large fraction of…

astro-ph.SR2020★ 76 cited

Long-term evolution of a magnetic massive merger product

F. R. N. Schneider, S. T. Ohlmann, Ph. Podsiadlowski +3

About 10% of stars more massive than ≈1.5M⊙​ have strong, large-scale surface magnetic fields and are being discussed as progenitors of highly-magnetic w…

astro-ph.SR2019

The MiMeS survey of Magnetism in Massive Stars: Magnetic properties of the O-type star population

V. Petit, G. A. Wade, F. R. N. Schneider +5

In this paper, we describe an analysis of the MiMeS Survey of O-type stars to explore the range of dipolar field strengths permitted by the polarisation spectra that do not yield a…

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