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Hannah E. Brinkman

3 papers here

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

author position
  • first author2
  • middle author1

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

fields
  • astro-ph.SR3
ORCID 0000-0002-7634-2432

identity via Semantic Scholar / OpenAlex

most citedThe Occurrence and Impact of Carbon-Oxygen Shell Mergers in Massive Stars

13 citations · 17 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2025★ 4 cited

Mixing due to internal gravity waves can explain the CNO surface abundances of B-type detached eclipsing binaries and single stars

Hannah E. Brinkman, Andrew Tkachenko, Conny Aerts

Observations of double-lined spectroscopic eclipsing binaries are ideal to study stellar evolution. They have tight model-independent constraints on their masses and radii. With th…

astro-ph.SR2025★ 13 cited

The Occurrence and Impact of Carbon-Oxygen Shell Mergers in Massive Stars

L. Roberti, M. Pignatari, H. E. Brinkman +6

In their final stages before undergoing a core-collapse supernova, massive stars may experience mergers between internal shells where carbon (C) and oxygen (O) are consumed as fuel…

astro-ph.SR2024

The impact of asteroseismically calibrated internal mixing on nucleosynthetic wind yields of massive stars

Hannah E. Brinkman, Lorenzo Roberti, Alex Kemp +3

Asteroseismology gives us the opportunity to look inside stars and determine their internal properties. Based on these observations, estimations can be made for the amount of the c…

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