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researcher

R. Edgar

19 papers hereh-index 143.7k citations32 works total

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

author position
  • sole author5
  • first author7
  • middle author3
  • last author3

Across the 18 of 19 papers where every author was matched, so the position is known.

fields
  • astro-ph14
  • astro-ph.IM3
  • astro-ph.SR2
same name
  • R. Edgar — 32 papers, h 61
  • R. Edgar — 17 papers, h 28
  • R. Edgar — 1 paper, h 2
  • R. Edgar — 1 paper, h 3

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

activity
20002011
most citedA comparative study of disc-planet interaction

446 citations · 1.2k across the 18 of their papers we have counts for

collaborators
Showing 2007Show all

4 papers · 1 filter

astro-ph2007★ 42 cited

The Formation of Crystalline Dust in AGB Winds from Binary Induced Spiral Shocks

R. G. Edgar, J. Nordhaus, E. Blackman +1

As stars evolve along the Asymptotic Giant Branch, strong winds are driven from the outer envelope. These winds form a shell, which may ultimately become a planetary nebula. Many p…

astro-ph2007★ 1 cited

Evidence for Growth of Eccentricity and Mass Clearing in a Disc Interior to a Planet

Richard G. Edgar, Eric Blackman, Alice Quillen +2

We present computational results showing eccentricity growth in the inner portions of a protoplanetary disc. We attribute this to the evolving surface density of the disc. The plan…

astro-ph2007★ 20 cited

The Minimum Gap-opening Planet Mass in an Irradiated Circumstellar Accretion Disk

Richard G. Edgar, Alice C. Quillen, Jaehong Park

We consider the minimum mass planet, as a function of radius, that is capable of opening a gap in an α-accretion disk. We estimate that a half Jupiter mass planet can open a gap…

astro-ph2007★ 43 cited

Giant Planet Migration in Viscous Power-Law Discs

R. G. Edgar

Many extra-solar planets discovered over the past decade are gas giants in tight orbits around their host stars. Due to the difficulties of forming these `hot Jupiters' in situ, th…

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