L
L. A. S. McClelland
Researcher at University of Auckland
Publications - 5
Citations - 1127
L. A. S. McClelland is an academic researcher from University of Auckland. The author has contributed to research in topics: Stellar evolution & Supernova. The author has an hindex of 3, co-authored 5 publications receiving 926 citations.
Papers
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Journal ArticleDOI
Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
John J. Eldridge,Elizabeth R. Stanway,L. Xiao,L. A. S. McClelland,G. Taylor,M. Ng,Stephanie M. L. Greis,J. C. Bray +7 more
TL;DR: The Binary Population and Spectral Synthesis suite of binary stellar evolution models and synthetic stellar populations provides a framework for the physically motivated analysis of both the integrated light from distant stellar populations and the detailed properties of those nearby as discussed by the authors.
Journal ArticleDOI
Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
John J. Eldridge,Elizabeth R. Stanway,L. Xiao,L. A. S. McClelland,G. Taylor,M. Ng,Stephanie M. L. Greis,J. C. Bray +7 more
TL;DR: The Binary Population and Spectral Synthesis (BPASS) suite of binary stellar evolution models and synthetic stellar populations provides a framework for the physically motivated analysis of both the integrated light from distant stellar populations and the detailed properties of those nearby as mentioned in this paper.
Journal ArticleDOI
Helium stars: towards an understanding of Wolf–Rayet evolution
TL;DR: In this article, a grid of pure helium star models is used to investigate how varying mass-loss rate affects the evolution of Wolf-Rayet (WR) stars, and it is shown that the temperature ranges of observed WR stars can be reproduced by varying the mass loss rate, which effectively determines the size of the helium envelope around the core.
Journal ArticleDOI
Binary Population and Spectral Synthesis
John J. Eldridge,Elizabeth R. Stanway,L. Xiao,L. A. S. McClelland,J. C. Bray,G. Taylor,M. Ng +6 more
TL;DR: The Binary Population and Spectral Synthesis (BPASS) as mentioned in this paper code is designed to construct the spectra and related properties of stellar populations built from ~200,000 detailed, individual stellar models of known age and metallicity.
Journal ArticleDOI
Helium Stars: Towards an Understanding of Wolf-Rayet Evolution
TL;DR: In this paper, a large grid of pure helium star models is used to investigate the dependence of the surface temperatures on factors such as the rate of mass loss and the amount of clumping in the outer convection zone.