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researcher

J. Fuller

15 papers hereh-index 572 citations19 works total

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

author position
  • first author3
  • middle author7
  • last author5

Across the 15 of 15 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE5
  • astro-ph.SR5
  • astro-ph.EP4
  • astro-ph.IM1
same name
  • J. Fuller — 110 papers, h 38
  • J. Fuller — 18 papers, h 2
  • J. Fuller — 12 papers, h 6
  • J. Fuller — 4 papers, h 24
  • J. Fuller — 3 papers, h 11
  • J. Fuller — 2 papers, h 1

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
20232026
most citedBoil-off of red supergiants: mass loss and type II-P supernovae

36 citations · 77 across the 15 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

4 papers · 1 filter

astro-ph.EP2026

Origin of Hyperion and Saturn's Rings in A Two-Stage Saturnian System Instability

Matija Ćuk, Maryame El Moutamid, Jim Fuller +1

The age of the rings and some of the moons of Saturn is an open question, and multiple lines of evidence point to a recent (few hundred Myr ago) cataclysm involving disruption of p…

astro-ph.EP2026

Excitation and Damping of Oscillation Modes in Gaseous Planets

Jim Fuller, Marzia Parisi, Steve Markham +2

The excitation and damping mechanisms for oscillation modes of gas giant planets are undetermined. We show that differential rotation may greatly enhance convective viscosity in gi…

astro-ph.EP2024

Tidal Dissipation in Giant Planets

Jim Fuller, Tristan Guillot, Stephane Mathis +1

Tidal interactions between moons and planets can have major effects on the orbits, spins, and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet…

astro-ph.EP2023

Tidal migration of exoplanets around M-dwarfs: frequency-dependent tidal dissipation

Samantha C. Wu, Janosz W. Dewberry, Jim Fuller

The orbital architectures of short-period exoplanet systems are shaped by tidal dissipation in their host stars. For low-mass M-dwarfs whose dynamical tidal response comprises a de…

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