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Stephen Ro

3 papers here

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

author position
  • sole author1
  • middle author2

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

fields
  • astro-ph.SR2
  • astro-ph.HE1
ORCID 0000-0001-6148-449X

identity via Semantic Scholar / OpenAlex

most citedOblique Shock Breakout in Supernovae and Gamma-Ray Bursts: II. Numerical Solutions For Non-Relativistic Pattern Speeds

18 citations · 47 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2019★ 14 cited

The Wolf-Rayet Stellar Response To The Iron Opacity Bump: Envelope Inflation, Winds, and Microturbulence

Stephen Ro

Early-type Wolf-Rayet(WR) stellar models harbor a super-Eddington layer in their outer envelopes due to a prominent iron opacity bump. In the past few decades, one-dimensional hydr…

astro-ph.HE2019★ 15 cited

Weak Shock Propagation with Accretion. II. Stability of Self-similar Solutions to Radial Perturbations

Eric R. Coughlin, Stephen Ro, Eliot Quataert

Coughlin et al. (2018) (Paper I) derived and analyzed a new regime of self-similarity that describes weak shocks (Mach number of order unity) in the gravitational field of a point…

astro-ph.SR2014★ 18 cited

Oblique Shock Breakout in Supernovae and Gamma-Ray Bursts: II. Numerical Solutions For Non-Relativistic Pattern Speeds

Pegah Salbi, Christopher D. Matzner, Stephen Ro +1

Non-spherical explosions develop non-radial flows as the pattern of shock emergence progresses across the stellar surface. In supernovae these flows can limit ejecta speeds, stifle…

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