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researcher

R. Smith

4 papers hereh-index 00 citations0 works total

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

author position
  • middle author3
  • last author1

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

fields
  • astro-ph.GA3
  • astro-ph.HE1
same name
  • R. Smith — 114 papers, h 76
  • R. Smith — 33 papers, h 30
  • R. Smith — 27 papers, h 38
  • R. Smith — 27 papers
  • R. Smith — 24 papers
  • R. Smith — 19 papers, h 13

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedThe width of Herschel filaments varies with distance

45 citations · 80 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2021★ 8 cited

GRB 191016A: A highly collimated gamma-ray burst jet with magnetised energy injection

M. Shrestha, I. A. Steele, S. Kobayashi +7

Long gamma-ray burst GRB 191016A was a bright and slow rising burst that was detected by the \textit{Swift} satellite and followed up by ground based Liverpool Telescope (LT). LT f…

astro-ph.GA2021★ 45 cited

The width of Herschel filaments varies with distance

G. V. Panopoulou, S. E. Clark, A. Hacar +5

Context: Filamentary structures in nearby molecular clouds have been found to exhibit a characteristic width of 0.1 pc, as observed in dust emission. Understanding the origin of th…

astro-ph.GA2021★ 16 cited

The "Maggie" filament: Physical properties of a giant atomic cloud

J. Syed, J. D. Soler, H. Beuther +19

The atomic phase of the interstellar medium plays a key role in the formation process of molecular clouds. Due to the line-of-sight confusion in the Galactic plane that is associat…

astro-ph.GA2016★ 11 cited

Could Segue 1 be a destroyed star cluster? - a dynamical perspective

Raul Dominguez, Michael Fellhauer, Matias Blaña +5

We attempt to find a progenitor for the ultra-faint object Segue 1 under the assumption that it formed as a dark matter free star cluster in the past. We look for orbits, using the…

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