S
Scott Tremaine
Researcher at Institute for Advanced Study
Publications - 259
Citations - 46961
Scott Tremaine is an academic researcher from Institute for Advanced Study. The author has contributed to research in topics: Galaxy & Planet. The author has an hindex of 90, co-authored 256 publications receiving 44123 citations. Previous affiliations of Scott Tremaine include Canadian Institute for Advanced Research & Princeton University.
Papers
More filters
Journal ArticleDOI
Comparison of approximately isothermal gravitational potentials of elliptical galaxies based on X-ray and optical data
E. M. Churazov,Scott Tremaine,William R. Forman,Ortwin Gerhard,Payel Das,Alexey Vikhlinin,C. Jones,Hans Böhringer,Karl Gebhardt +8 more
TL;DR: In this paper, the authors analyzed six X-ray bright elliptical galaxies, observed with Chandra and XMM-Newton, and approximate their gravitational potentials by isothermal spheres ϕ =v 2c logr over a range of radii from ∼ 0.5 to ∼ 25 kpc.
Journal ArticleDOI
Gauss's method for secular dynamics, softened
TL;DR: Fabrycky et al. as mentioned in this paper, 2007, ASTROPHYS J, V669, P1298, DOI 10.1086-521702; Ford EB, 2000, AstropHys J,V542, P143, DOI10.1365-2966.
Journal ArticleDOI
On the Origin of Irregular Structure in Saturn's Rings
TL;DR: In this article, the Cahn-Hilliard equation was used to model the formation of ring particle assemblies in the B ring of Saturn's B ring, which is consistent with the sticking forces observed in laboratory simulations of frosted ice particles.
Journal ArticleDOI
Planets Near Mean-Motion Resonances
TL;DR: In this paper, a simple dynamical model for planet formation was proposed, in which planets grow in mass at a prescribed rate without orbital migration or dissipation, and the observed peak-trough structure was verified with numerical integrations of the restricted three-body problem.
Journal ArticleDOI
Towards a theory for Neptune's arc rings
TL;DR: In this article, it was shown that the incomplete rings of Neptune consist of a number of short arcs centered on the corotation resonances of a single satellite, and the estimated surface mass densities are comparable to those found in the major rings of Saturn and Uranus.