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Cited by 273

The DOI matches its Crossref record; 27 of the 27 references it cites were found in a registry or an index.

Does the Fornax dwarf spheroidal have a central cusp or core?

Open access
Goerdt, Tobias, Moore, Ben, Read, J. I., Stadel, Joachim, Zemp, Marcel·2006·Monthly Notices of the Royal Astronomical Society

Abstract

The dark matter dominated Fornax dwarf spheroidal has five globular clusters orbiting at ∼1 kpc from its centre. In a cuspy cold dark matter halo the globulars would sink to the centre from their current positions within a few Gyr, presenting a puzzle as to why they survive undigested at the present epoch. We show that a solution to this timing problem is to adopt a cored dark matter halo. We use numerical simulations and analytic calculations to show that, under these conditions, the sinking time becomes many Hubble times; the globulars effectively stall at the dark matter core radius. We conclude that the Fornax dwarf spheroidal has a shallow inner density profile with a core radius constrained by the observed positions of its globular clusters. If the phase space density of the core is primordial then it implies a warm dark matter particle and gives an upper limit to its mass of ∼0.5 keV, consistent with that required to significantly alleviate the substructure problem.

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Metadata

Authors
Goerdt, T., Moore, B., Read, J. I., Stadel, J., & Zemp, M.
Venue
Monthly Notices of the Royal Astronomical Society
Published
2006-04-13
Volume
368
Issue
3
Pages
1073-1077
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2014602460
Cited by
273
References
27
FWCI
14.27
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Does the Fornax dwarf spheroidal have a central cusp or core? https://app.cochat.ai/papers/10.1111/j.1365-2966.2006.10182.x
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Goerdt, T., Moore, B., Read, J. I., Stadel, J., & Zemp, M. (2006). Does the Fornax dwarf spheroidal have a central cusp or core? Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2006.10182.x

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