N
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
The Optical Structure of the Starburst Galaxy M82. II. Nebular Properties of the Disk and Inner-Wind
M. S. Westmoquette,John S. Gallagher,Linda J. Smith,Linda J. Smith,G. Trancho,Nate Bastian,Iraklis S. Konstantopoulos +6 more
TL;DR: In this paper, the results from optical Gemini-North GMOS-IFU and WIYN DensePak spectroscopic observations of the starburst and inner wind zones of M82, with a focus on the state of the T~10^4 K ionized interstellar medium.
Posted Content
Looking for Systematic Variations in the Stellar Initial Mass Function
TL;DR: In this paper, a critical look at the case for IMF variations, with a view towards whether other explanations are sufficient given the evidence, is taken, and it is shown that the vast majority of the observed stellar populations are drawn from a universal initial mass function.
Book ChapterDOI
Star Clusters in Interacting Galaxies: The Case of M51
TL;DR: In this paper, the spectral energy distribution (SED) of stellar clusters in the interacting galaxy, M51, using HST-WFPC2 observations was compared with those of evolutionary spectral synthesis models, derived an age, mass, and extinction for each source.
Book ChapterDOI
Star Clusters in Interacting Galaxies: The Case of M51
TL;DR: In this article, the spectral energy distribution (SED) of stellar clusters in the interacting galaxy, M51, using HST-WFPC2 observations was compared with those of evolutionary spectral synthesis models, derived an age, mass, and extinction for each source.
Looking for Systematic Variations in the Stellar Initial Mass Function
TL;DR: In this article, a critical look at the case for IMF variations, with a view towards whether other explanations are sufficient given the evidence, is taken, and it is shown that the vast majority of the observed stellar populations are drawn from a universal initial mass function.