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S. Peng Oh

3 papers here

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

author position
  • middle author3

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

fields
  • astro-ph2
  • astro-ph.CO1
ORCID 0000-0002-1013-4657

identity via Semantic Scholar / OpenAlex

most citedEarly Cosmological HII/HeIII Regions and Their Impact on Second-Generation Star Formation

208 citations · 347 across the 3 of their papers we have counts for

collaborators
Showing astro-phShow all

2 papers · 1 filter

astro-ph2006★ 208 cited

Early Cosmological HII/HeIII Regions and Their Impact on Second-Generation Star Formation

Naoki Yoshida, S. Peng Oh, Tetsu Kitayama +1

(Abridged) We present the results of three-dimensional radiation-hydrodynamics simulations of the formation and evolution of early HII/HeIII regions around the first stars. Cooling…

astro-ph2006★ 126 cited

The Effects of Dark Matter Decay and Annihilation on the High-Redshift 21 cm Background

Steven Furlanetto, S. Peng Oh, Elena Pierpaoli

The radiation background produced by the 21 cm spin-flip transition of neutral hydrogen at high redshifts can be a pristine probe of fundamental physics and cosmology. At z~30-300,…

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