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P. Ou 歐

3 papers hereh-index 343 citations8 works total

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.HE2
  • astro-ph.SR1

identity via Semantic Scholar / OpenAlex

activity
20182026
collaborators

3 papers

astro-ph.HE2026

Multi-wavelength Signatures of Supernova Shock Breakout from Red Supergiants in Two Dimensions

Wun-Yi Chen, Ke-Jung Chen, Keiichi Maeda +3

We present new two-dimensional radiation hydrodynamic simulations of supernova shock breakout from red supergiants using the CASTRO code. Our progenitors are 20 and 25 M…

astro-ph.SR2025

Critical Metallicity of Cool Supergiant Formation. II. Physical Origin

Po-Sheng Ou, Ke-Jung Chen

This study investigates the physical origin of the critical metallicity required for the formation of cool supergiants, as revealed by stellar evolution models. Using grids of stel…

astro-ph.HE2018

X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC

Po-Sheng Ou, You-Hua Chu, Pierre Maggi +3

The Large Magellanic Cloud (LMC) has ∼60 confirmed supernova remnants (SNRs). Because of the known distance, 50 kpc, the SNRs' angular sizes can be converted to linear sizes,…

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