activity
20082023
most citedBuilding up the Population III initial mass function from cosmological initial conditions

256 citations · 615 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2023★ 3 cited

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A forming quadruple system with continuum `ribbons' and intricate outflows

Qiu-yi Luo, Tie Liu, Aaron T. Lee +31

One of the most poorly understood aspects of low-mass star formation is how multiple-star systems are formed. Here we present the results of Atacama Large Millimeter/submillimeter…

astro-ph.CO2022★ 36 cited

Magnetic fields in the formation of the first stars.--II Results

Athena Stacy, Christopher F. McKee, Aaron T. Lee +2

Beginning with cosmological initial conditions at z=100, we simulate the effects of magnetic fields on the formation of Population III stars and compare our results with the predic…

astro-ph.GA2020★ 22 cited

The highly variable time evolution of star-forming cores identified with dendrograms

Rachel A. Smullen, Kaitlin M. Kratter, Stella S. R. Offner +2

We investigate the time evolution of dense cores identified in molecular cloud simulations using dendrograms, which are a common tool to identify hierarchical structure in simulati…

astro-ph.GA2019★ 74 cited

The Formation and Evolution of Wide-Orbit Stellar Multiples In Magnetized Clouds

Aaron T. Lee, Stella S. R. Offner, Kaitlin M. Kratter +2

Stars rarely form in isolation. Nearly half of the stars in the Milky Way have a companion, and this fraction increases in star-forming regions. However, why some dense cores and f…

astro-ph.IM2016★ 43 cited

Hybrid Adaptive Ray-Moment Method (HARM): A Highly Parallel Method for Radiation Hydrodynamics on Adaptive Grids

Anna L. Rosen, Mark R. Krumholz, Jeffrey S. Oishi +2

We present a highly-parallel multi-frequency hybrid radiation hydrodynamics algorithm that combines a spatially-adaptive long characteristics method for the radiation field from po…

astro-ph.GA2016★ 256 cited

Building up the Population III initial mass function from cosmological initial conditions

Athena Stacy, Volker Bromm, Aaron T. Lee

We simulate the growth of a Population III stellar system, starting from cosmological initial conditions at z=100. We follow the formation of a minihalo and the subsequent collapse…