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Breaking beta: a comparison of mass modelling methods for spherical systems
External Source
chorus
Document Type
Version of Record
Authors
J I Read (Department of Physics, University of Surrey, Guildford GU2 7XH, UK)
G A Mamon (Institut d’Astrophysique de Paris (UMR 7095: CNRS & Sorbonne Université), F-75014 Paris, France)
E Vasiliev (Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK)
L L Watkins (AURA for the European Space Agency (ESA), ESA Office, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA)
M G Walker (McWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213, USA)
J Peñarrubia (Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK)
M Wilkinson (Department of Physics & Astronomy, University of Leicester, Leicester LE1 7RH, UK)
W Dehnen (Department of Physics & Astronomy, University of Leicester, Leicester LE1 7RH, UK)
P Das (Department of Physics, University of Surrey, Guildford GU2 7XH, UK)
Date Acquired
February 10, 2025
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 501
Issue: 1
ISSN: 0035-8711
e-ISSN: 1365-2966
DOI: 10.1093/mnras/staa3663
Funding Number(s)
funding: ST/M000990/1
funding: 321067
funding: AR-14322
Distribution Limits
Public

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