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S. Ohlmann

12 papers hereh-index 211.8k citations48 works total

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

author position
  • middle author10

Across the 10 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR7
  • astro-ph.HE3
  • cond-mat.mes-hall1
  • physics.comp-ph1

identity via Semantic Scholar / OpenAlex

activity
20152024
most citedHow mergers magnetise massive stars

270 citations · 622 across the 7 of their papers we have counts for

collaborators
Showing 2020Show all

4 papers · 1 filter

astro-ph.SR2020

Common-envelope evolution with an asymptotic giant branch star

C. Sand, S. T. Ohlmann, F. R. N. Schneider +2

Common-envelope phases are decisive for the evolution of many binary systems. Of particular interest are cases with asymptotic giant branch (AGB) primary stars, because they are th…

astro-ph.SR2020

Formation of sdB-stars via common envelope ejection by substellar companions

M. Kramer, F. R. N. Schneider, S. T. Ohlmann +4

Common envelope (CE) phases in binary systems where the primary star reaches the tip of the red giant branch are discussed as a formation scenario for hot subluminous B-type (sdB)…

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.SR2020

SNe Ia from double detonations: Impact of core-shell mixing on the carbon ignition mechanism

Sabrina Gronow, Christine Collins, Sebastian T. Ohlmann +5

Sub-Chandrasekhar mass white dwarfs accreting a helium shell on a carbon-oxygen core are potential progenitors of normal Type Ia supernovae. This work focuses on the details of the…

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