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Nate Bastian
Researcher at Liverpool John Moores University
Publications - 365
Citations - 20094
Nate Bastian is an academic researcher from Liverpool John Moores University. The author has contributed to research in topics: Galaxy & Star cluster. The author has an hindex of 76, co-authored 355 publications receiving 18342 citations. Previous affiliations of Nate Bastian include University of Exeter & Technische Universität München.
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Journal ArticleDOI
Erratum: "The Rotating Nuclear Star Cluster in NGC 4244" (2008, ApJ, 687, 997)
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Young Massive Clusters: Their Population Properties, Formation and Evolution, and Their Relation to the Ancient Globular Clusters
TL;DR: In this article, the main properties of Young Massive Clusters (YMCs) including their population properties, including luminosity, mass and age distributions of the clusters, were discussed.
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New results on the ages of star clusters in region B of M82
Iraklis S. Konstantopoulos,Nate Bastian,Linda J. Smith,Linda J. Smith,Gelys Trancho,M. S. Westmoquette,Jay Gallagher +6 more
TL;DR: In this article, the authors present Gemini-North optical spectra of seven star clusters in M82-B and show that their ages are all between 10 and 300 myr (a factor of 3-100 younger than previous photometric results).
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What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
Meghan E Hughes,Prashin Jethwa,Michael Hilker,Glenn van de Ven,Marie Martig,Joel Pfeffer,Nate Bastian,J. M. Diederik Kruijssen,Sebastian Trujillo-Gomez,Marta Reina-Campos,Robert A. Crain +10 more
TL;DR: In this paper, the authors used the E-MOSAICS suite of 25 zoom-in simulations of L * galaxies to test the performance of Jeans-Anisotropic-MGE (JAM) models using Globular Clusters (GCs) as tracers.
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Dynamical Masses of Young Star Clusters: Constraints on the Stellar IMF and Star-Formation Efficiency
Nate Bastian,Simon P. Goodwin +1 more
TL;DR: In this article, it was shown that only the older clusters are suitable for IMF studies and the younger clusters can be used instead to constrain the star-formation efficiency (SFE) within clusters, and that approximately 60% of young clusters are unbound and will not survive for more than a few 10's of Myr.