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Stephen D. Murray

4 papers hereh-index 3139 citations3 works total

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

author position
  • middle author1
  • last author3

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.GA1

identity via Semantic Scholar / OpenAlex

activity
20002014
most citedMagnetohydrodynamic Simulations of Shock Interactions with Radiative Clouds

74 citations · 136 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2014★ 1 cited

Update on 3D Moving Mesh Simulations of Galactic Center Cloud G2

P. Chris Fragile, Peter Anninos, Stephen D. Murray

Using three-dimensional, moving-mesh simulations, we investigate the future evolution of the recently discovered gas cloud G2 traveling through the galactic center. From our simula…

astro-ph2004★ 74 cited

Magnetohydrodynamic Simulations of Shock Interactions with Radiative Clouds

P. Chris Fragile, Peter Anninos, Kyle Gustafson +1

We present results from two-dimensional numerical simulations of the interactions between magnetized shocks and radiative clouds. Our primary goal is to characterize the dynamical…

astro-ph2004★ 33 cited

Ejection of Supernova-Enriched Gas From Dwarf Disk Galaxies

P. Chris Fragile, Stephen D. Murray, Douglas N. C. Lin

We examine the efficiency with which supernova-enriched gas may be ejected from dwarf disk galaxies, using a methodology previously employed to study the self-enrichment efficiency…

astro-ph2000★ 28 cited

On the Two-Phase Structure of Protogalactic Clouds

D. N. C. Lin, S. D. Murray

Within protogalaxies, thermal instability leads to the formation of a population of cool fragments, confined by the pressure of residual hot gas. The hot gas remains in quasi-hydro…

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