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The WAGGS project-III. Discrepant mass-to-light ratios of Galactic globular clusters at high metallicity
External Source
chorus
Document Type
Version of Record
Authors
H Dalgleish (Astrophysics Research Institute, Liverpool John Moores University, Liverpool, L3 5RF, UK)
S Kamann (Astrophysics Research Institute, Liverpool John Moores University, Liverpool, L3 5RF, UK)
C Usher (Astrophysics Research Institute, Liverpool John Moores University, Liverpool, L3 5RF, UK)
H Baumgardt (School of Mathematics and Physics, The University of Queensland, St. Lucia, QLD 4072, Australia)
N Bastian (Astrophysics Research Institute, Liverpool John Moores University, Liverpool, L3 5RF, UK)
J Veitch-Michaelis (Astrophysics Research Institute, Liverpool John Moores University, Liverpool, L3 5RF, UK)
A Bellini (Space Telescope Science Institute, 3800 San Martin Drive, Baltimore, MD 21218, USA)
S Martocchia (Astrophysics Research Institute, Liverpool John Moores University, Liverpool, L3 5RF, UK)
G S Da Costa (Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia)
D Mackey (Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia)
S Bellstedt (ICRAR, The University of Western Australia, 7 Fairway, Crawley WA 6009, Australia)
N Pastorello (BlueScope, Level 11, 120 Collins Street, Melbourne VIC 3000, Australia)
P Cerulo (Department of Astronomy, Universidad de Concepción, Casilla 160-C, Concepción, Chile)
Date Acquired
October 21, 2024
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 492
Issue: 3
Issue Publication Date: January 3, 2020
ISSN: 0035-8711
e-ISSN: 1365-2966
DOI: 10.1093/mnras/staa091
Funding Number(s)
funding: 31180051
funding: NAS 5-26555
Distribution Limits
Public

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