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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.
Papers
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Journal ArticleDOI
An alternative method to study star cluster disruption
Mark Gieles,Nate Bastian +1 more
TL;DR: In this paper, the authors introduced a new method based on size-of-sample effects, namely the relation between the most massive cluster, M_max, and the age range sampled, such that the slope in a log(M_max) vs. log(age) plot is equal to unity.
Journal ArticleDOI
Exploring the role of binarity in the origin of the bimodal rotational velocity distribution in stellar clusters
Sebastian Kamann,Nate Bastian,Nate Bastian,Nate Bastian,Christopher Usher,I. Cabrera-Ziri,I. Cabrera-Ziri,S. Saracino +7 more
TL;DR: In this paper, the binary channel was used to search for differences in the binary fraction of the slow and fast rotating populations of NGC 1850, a 100Myr massive cluster in the LMC.
Posted Content
Cluster Disruption: From infant mortality to long term survival
TL;DR: In this paper, the authors review the theory and observations of cluster disruption, both the suggested initial rapid dissolution phase (infant mortality) and the longer timescale processes that affect clusters after they emerge from their progenitor GMCs.
Journal ArticleDOI
Searching for multiple populations in the integrated light of the young and extremely massive clusters in the merger remnant NGC 7252
Nate Bastian,Carmela Lardo,Christopher Usher,Sebastian Kamann,Søren S. Larsen,I. Cabrera-Ziri,W. Chantereau,S. Martocchia,S. Martocchia,Maurizio Salaris,Randa Asa'd,Michael Hilker +11 more
TL;DR: In this article, the presence or absence of multiple populations using integrated light spectroscopy of the W3 and W30 massive stellar clusters in the galactic merger remnant, NGC 7252, was investigated.
Book ChapterDOI
The Radii of Thousands of Star Clusters in M51 with HST/ACS
TL;DR: In this article, the authors exploit the superb resolution of the new HST/ACS mosaic image of M51 to select a large sample of young star clusters in the spiral disk, based on their sizes.