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Samantha Wu

3 papers here

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

author position
  • middle author2
  • last author1

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

fields
  • astro-ph.SR2
  • astro-ph.HE1
ORCID 0000-0003-2872-5153

identity via Semantic Scholar / OpenAlex

activity
20232025
most citedOn the damping of tidally driven oscillations

6 citations · 8 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2025

A Spectroscopic Hunt for Post-Red Supergiants in the Large Magellanic Cloud II: Turbulent Line Broadening in the Spectra of LMC Yellow Supergiants

Trevor Z. Dorn-Wallenstein, Kaitlyn M. Chen, Samantha C. Wu +4

Massive stars in the Hertzsprung gap are a mixed population of objects in short-lived evolutionary phases: yellow supergiants (YSGs) evolving towards the red supergiant (RSG) phase…

astro-ph.HE2024★ 2 cited

Bright Supernova Precursors by Outbursts from Massive Stars with Compact Object Companions

Daichi Tsuna, Tatsuya Matsumoto, Samantha C. Wu +1

A fraction of core-collapse supernovae (SNe) with signs of interaction with a dense circumstellar matter are preceded by bright precursor emission. While the precursors are likely…

astro-ph.SR2023★ 6 cited

On the damping of tidally driven oscillations

Janosz W. Dewberry, Samantha C. Wu

Expansions in the oscillation modes of tidally perturbed bodies provide a useful framework for representing tidally induced flows. However, recent work has demonstrated that such e…

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