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Alan P. Boss

Researcher at Carnegie Institution for Science

Publications -  431
Citations -  40212

Alan P. Boss is an academic researcher from Carnegie Institution for Science. The author has contributed to research in topics: Planet & Formation and evolution of the Solar System. The author has an hindex of 78, co-authored 426 publications receiving 38471 citations. Previous affiliations of Alan P. Boss include Ames Research Center & NASA Headquarters.

Papers
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Tidal disruption of inviscid planetesimals

TL;DR: In this article, the smooth particle hydrodynamics (SPH) code of Cameron and Benz (1991) was used to simulate the impact of 0.01 earth-mass planetesimals passing by the earth with variations in the impact parameter at perigee and velocity at infinity.
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Supernova-triggered molecular cloud core collapse and the rayleigh-taylor fingers that polluted the solar nebula

TL;DR: In this paper, the authors used the FLASH adaptive mesh refinement hydrodynamics code to calculate the first fully three-dimensional (3D) models of the triggering and injection process.
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A keck hires doppler search for planets orbiting metal-poor dwarfs. i. testing giant planet formation and migration scenarios

TL;DR: In this article, a high-precision Doppler search for giant planets orbiting a well-defined sample of metal-poor dwarfs in the field is described, which constitutes a fundamental test of theoretical predictions, which will help discriminate between proposed giant planetformationand migrationmodels.
Book

The astrophysics of planetary systems : formation, structure, and dynamical evolution : proceedings of the 276th Symposium of the International Astronomical Union, held in Torino, Italy, October 10-15, 2010

TL;DR: In this paper, the authors discuss the next decade in the field of Planet Formation, Structure and Atmospheres, Interactions, and the Next Decade Part V. Poster Papers.
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New Parallaxes and a Convergence Analysis for the TW Hya Association

TL;DR: The TW Hya Association (TWA) is a nearby stellar association with an age of 5-10 Myr as mentioned in this paper, which is an important age for studying the late stages of star and planet formation.