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19972005
most citedStellar Collisions and the Interior Structure of Blue Stragglers

160 citations · 602 across the 7 of their papers we have counts for

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astro-ph2005★ 94 cited

Blue Stragglers as Stellar Collision Products: the Angular Momentum Question

Alison Sills, Tim Adams, Melvyn B. Davies

We investigate the structure and evolution of blue stragglers stars which were formed from direct stellar collisions between main sequence stars in globular clusters. In particular…

astro-ph2001★ 160 cited

Stellar Collisions and the Interior Structure of Blue Stragglers

James C. Lombardi, Jessica Sawyer Warren, Frederic A. Rasio +2

Collisions of main sequence stars occur frequently in dense star clusters. In open and globular clusters, these collisions produce merger remnants that may be observed as blue stra…

astro-ph1998★ 76 cited

Tests of Spurious Transport in Smoothed Particle Hydrodynamics

James C. Lombardi, Alison Sills, Frederic A. Rasio +1

We have performed a series of systematic tests to evaluate the effects of spurious transport in three-dimensional smoothed particle hydrodynamics (SPH) calculations. Our tests inve…

astro-ph1998★ 82 cited

Structure and Evolution of Nearby Stars with Planets. I. Short-Period Systems

Eric B. Ford, Frederic A. Rasio, Alison Sills

Using the Yale stellar evolution code, we have calculated theoretical models for nearby stars with planetary-mass companions in short-period nearly circular orbits: 51 Pegasi, Tau…

astro-ph1998★ 56 cited

The Distribution of Collisionally Induced Blue Stragglers in the Colour-Magnitude Diagram

Alison Sills, Charles D. Bailyn

A primary production mechanism for blue stragglers in globular clusters is thought to be collisionally-induced mergers, perhaps mediated by dynamical encounters involving binary st…

astro-ph1997★ 28 cited

The Importance of Realistic Starting Models for Hydrodynamic Simulations of Stellar Collisions

Alison Sills, James C. Lombardi

We demonstrate the necessity of using realistic stellar models taken from stellar evolution codes, as opposed to polytropes, for starting models in smoothed particle hydrodynamics…