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researcher

Patrick Eggenberger

7 papers hereh-index 15 citations7 works total

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

author position
  • middle author6
  • last author1

Across the 7 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP4
  • astro-ph.SR3
same name
  • Patrick Eggenberger — 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
20222026
most citedAngular momentum transport near convective-core boundaries of Gamma Doradus stars

12 citations · 26 across the 7 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2026

The Beauty of k2: Probing Stellar Interiors Using Apsidal Motion. I. The Benchmark Massive Binary HD 152248

Sophie Rosu, Luca Sciarini, Sylvia Ekström +4

Over the last decades, several independent studies have shown the need for large convective boundary mixing (CBM) and convective core sizes in massive stars to reproduce a variety…

astro-ph.SR2026★ 1 cited

On the origin of the rotation of massive stars

André Oliva, Facundo D. Moyano, Luca Sciarini +3

We explore the origin of the rotation rates of massive stars. Contrary to their low-mass siblings, most massive stars do not have detectable magnetic fields, so that star-disk inte…

astro-ph.SR2024★ 12 cited

Angular momentum transport near convective-core boundaries of Gamma Doradus stars

Facundo Moyano, Patrick Eggenberger, Sébastien Salmon

Recent asteroseismic studies have revealed that the convective core of γ Doradus stars rotates faster than their radiative interior. We study the development of differential rota…

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