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Edward W. Thommes

2 papers here

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author position
  • first author1
  • middle author1

Across the 2 of 2 papers where every author was matched, so the position is known.

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  • astro-ph2
ORCID 0000-0001-6800-2000

identity via Semantic Scholar / OpenAlex

most citedDynamical Shakeup of Planetary Systems II. N-body simulations of Solar System terrestrial planet formation induced by secular resonance sweeping

81 citations · 102 across the 2 of their papers we have counts for

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Showing astro-phShow all

3 papers · 1 filter

astro-ph2008★ 81 cited

Dynamical Shakeup of Planetary Systems II. N-body simulations of Solar System terrestrial planet formation induced by secular resonance sweeping

E. W. Thommes, M. Nagasawa, D. N. C. Lin

We revisit the "dynamical shakeup" model of Solar System terrestrial planet formation, wherein the whole process is driven by the sweeping of Jupiter's secular resonance as the gas…

astro-ph2008★ 21 cited

Resonance Trapping in Protoplanetary Disks. I. Coplanar Systems

Aaron T. Lee, Edward W. Thommes, Frederic A. Rasio

Mean-motion resonances (MMRs) are likely to play an important role both during and after the lifetime of a protostellar gas disk. We study the dynamical evolution and stability of…

astro-ph2006★ 45 cited

Giant Planet Accretion and Migration: Surviving the Type I Regime

Edward W. Thommes, Norman Murray

In the standard model of gas giant planet formation, a large solid core (~ 10 times the Earth's mass) forms first, then accretes its massive envelope (100 or more Earth masses) of…

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