Search Results - "HosekJr, M. W"
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Stellar Populations in the Central 0.5 pc of Our Galaxy III: The Dynamical Sub-structures
Published 04-02-2023“…We measure the 3D kinematic structures of the young stars within the central 0.5 parsec of our Galactic Center using the 10 m telescopes of the W.~M.~Keck…”
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SPISEA: A Python-Based Simple Stellar Population Synthesis Code for Star Clusters
Published 10-07-2020“…We present SPISEA (Stellar Population Interface for Stellar Evolution and Atmospheres), an open-source Python package that simulates simple stellar…”
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Star Formation in Different Environments: The Initial Mass Function
Published 12-03-2019“…The stellar initial mass function (IMF) is a fundamental property of star formation, offering key insight into the physics driving the process as well as…”
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The Galactic Center: An Improved Astrometric Reference Frame for Stellar Orbits around the Supermassive Black Hole
Published 24-01-2019“…Precision measurements of the stars in short-period orbits around the supermassive black hole at the Galactic Center are now being used to constrain general…”
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The Unusual Initial Mass Function of the Arches Cluster
Published 02-11-2018“…As a young massive cluster in the Central Molecular Zone, the Arches cluster is a valuable probe of the stellar Initial Mass Function (IMF) in the extreme…”
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Consistency of the Infrared Variability of Sgr A over 22 years
Published 21-08-2019“…We report new infrared measurements of the supermassive black hole at the Galactic Center, Sgr A*, over a decade that was previously inaccessible at these…”
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The Galactic Center: Improved Relative Astrometry for Velocities, Accelerations, and Orbits near the Supermassive Black Hole
Published 07-02-2019“…We present improved relative astrometry for stars within the central half parsec of our Galactic Center based on data obtained with the 10 m W. M. Keck…”
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The Optical/Near-Infrared Extinction Law In Highly Reddened Regions
Published 25-01-2018“…A precise extinction law is a critical input when interpreting observations of highly reddened sources such as young star clusters and the Galactic Center…”
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