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19992026
most citedStructure and Evolution of Nearby Stars with Planets II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog

367 citations · 6.1k across the 116 of their papers we have counts for

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Showing astro-ph.GAShow all

42 papers · 1 filter

astro-ph.GA2024★ 1 cited

Dynamics of Star Cluster Formation: Mergers in Gas Rich Environments

Jeremy Karam, Alison Sills

We perform high resolution simulations of forming star clusters as they merge inside giant molecular clouds (GMCs) using hydrodynamics coupled to N-body dynamics to simultaneously…

astro-ph.GA2023★ 3 cited

Galactic properties that favour star cluster formation: a statistical view

Samantha C. Berek, Marta Reina-Campos, Gwendolyn Eadie +1

The presence or absence of star clusters in galaxies, and the properties of star cluster populations compared to their host galaxy properties, are important observables for validat…

astro-ph.GA2023★ 7 cited

Initial sizes of star clusters: implications for cluster dissolution during galaxy evolution

Marta Reina-Campos, Alison Sills, Godefroy Bichon

Massive star clusters are often used as tracers of galaxy formation and assembly. In order to do so, we must understand their properties at formation, and how those properties chan…

astro-ph.GA2023★ 7 cited

Modelling Star Cluster Formation: Gas Accretion

Jeremy Karam, Alison Sills

The formation of star clusters involves the growth of smaller, gas-rich subclusters through accretion of gas from the giant molecular cloud within which the subclusters are embedde…

astro-ph.GA2023★ 22 cited

Early Evolution and 3D Structure of Embedded Star Clusters

Claude Cournoyer-Cloutier, Alison Sills, William E. Harris +8

We perform simulations of star cluster formation to investigate the morphological evolution of embedded star clusters in the earliest stages of their evolution. We conduct our simu…

astro-ph.GA2022★ 3 cited

Using Molecular Gas Observations to Guide Initial Conditions for Star Cluster Simulations

Alison Sills, Steven Rieder, Anne S. M. Buckner +3

The earliest evolution of star clusters involves a phase of co-existence of both newly-formed stars, and the gas from which they are forming. Observations of the gas in such region…