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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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Probing the role of the galactic environment in the formation of stellar clusters, using M83 as a test bench
TL;DR: In this paper, a study of the M83 cluster population, covering the disc of the galaxy between radii of 0.45 and 4.5 kpc, is presented.
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Clusters in the inner spiral arms of M51: the cluster IMF and the formation history
TL;DR: In this article, the authors studied the cluster population in a region of 3.2x3.2 kpc^2 in the inner spiral arms of the intergacting galaxy M51, at a distance of about 1 to 3 kpc from the nucleus, based on HST-WFPC2 images taken through five broadband and two narrowband filters.
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Stellar clusters in M83: formation, evolution, disruption and the influence of the environment
Nate Bastian,Angela Adamo,Mark Gieles,E. Silva-Villa,H. J. G. L. M. Lamers,S. S. Larsen,Linda J. Smith,I. S. Konstantopoulos,Erik Zackrisson +8 more
TL;DR: In this article, the stellar cluster population in two adjacent fields in the nearby face-on spiral galaxy M83 was studied using multiwavelength Wide Field Camera 3/Hubble Space Telescope imaging.
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The dynamical mass of the young cluster W3 in NGC 7252. Heavy-weight globular cluster or ultra compact dwarf galaxy?
Claudia Maraston,Nate Bastian,Nate Bastian,Roberto P. Saglia,Markus Kissler-Patig,Francois Schweizer,Paul Goudfrooij +6 more
TL;DR: In this article, the authors determined the dynamical mass of the most luminous stellar cluster known to date, i.e. object W3 in the merger remnant galaxy NGC 7252.
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The luminosity function of young star clusters: implications for the maximum mass and luminosity of clusters
TL;DR: In this paper, a method to relate a possible truncation of the star cluster mass function at the high mass end to the shape of the cluster luminosity function (LF) was introduced.