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Rotation curves of galaxies and the stellar mass-to-light ratio

  • Published:2018-03-03 Issue:3 Volume:477 Page:4187-4199
  • ISSN:0035-8711
  • Container-title:Monthly Notices of the Royal Astronomical Society
  • language:en
  • Short-container-title:

Author:

Haghi Hosein1,Khodadadi Aziz1,Ghari Amir1,Zonoozi Akram Hasani1,Kroupa Pavel23

Affiliation:

1. Department of Physics, Institute for Advanced Studies in Basic Sciences (IASBS), PO Box 11365-9161, Zanjan, Iran

2. Helmholtz-Institut für Strahlen-und Kernphysik (HISKP), Universität Bonn, Nussallee 14-16, D-53115 Bonn, Germany

3. Faculty of Mathematics and Physics, Astronomical Institute, Charles University in Prague, V Holešovičkách 2, CZ-180 00 Praha 8, Czech Republic

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. A phenomenological model for dark matter phase-space distribution;Monthly Notices of the Royal Astronomical Society;2024-03-06

2. The Cusp–Core Problem in Gas-Poor Dwarf Spheroidal Galaxies;Galaxies;2021-12-30

3. Uncertainties in galaxy rotation curves;Monthly Notices of the Royal Astronomical Society;2021-01-06

4. Dark Matters on the Scale of Galaxies;Universe;2020-08-01

5. A 5° × 5° deep H i survey of the M81 group − II. H i distribution and kinematics of IC 2574 and HIJASS J1021+68;Monthly Notices of the Royal Astronomical Society;2020-02-12
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