Fornax globular cluster distributions: implications for the cusp-core problem-Reference-Cited by-同舟云学术

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Fornax globular cluster distributions: implications for the cusp-core problem

Published:2019-02-28 Issue:2 Volume:485 Page:2546-2557
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Boldrini Pierre¹,Mohayaee Roya¹,Silk Joseph¹²³

Affiliation:

1. Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris, 98 bis bd Arago, F-75014 Paris, France

2. Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218, USA

3. Department of Physics, Beecroft Institute for Particle Astrophysics and Cosmology, University of Oxford, Oxford OX1 3RH, UK

Funder

Horizon 2020

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/485/2/2546/28030656/stz573.pdf

Reference72 articles.

1. The core size of the Fornax dwarf spheroidal

2. Globular clusters as tracers of the host galaxy mass distribution: the Fornax dSph test case

3. Lack of nuclear clusters in dwarf spheroidal galaxies: implications for massive black holes formation and the cusp/core problem

4. Internal kinematics and dynamical models of dwarf spheroidal galaxies around the Milky Way

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4. The spatial distribution of globular clusters in dwarf spheroidal galaxies and the timing problem;Monthly Notices of the Royal Astronomical Society;2022-01-28

5. Can tides explain the low dark matter density in Fornax?;Monthly Notices of the Royal Astronomical Society;2021-12-08

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