Results 11 to 20 of about 601,655 (181)

A too-many dwarf satellite galaxies problem in the MATLAS low-to-moderate density fields [PDF]

open access: greenAstronomy & Astrophysics
Context.Dwarf galaxy abundances can serve as discernment tests for models of structure formation. Previous small-scale tensions between observations and dark matter-only cosmological simulations may have been resolved with the inclusion of baryonic processes; however, these successes have been largely concentrated on the Local Group dwarfs the feedback
Kosuke Jamie Kanehisa   +3 more
semanticscholar   +6 more sources

Inflation and the dwarf galaxy problem [PDF]

open access: greenPhysical Review D, 2000
Cosmological N-body simulations with scale-invariant initial perturbations show too many virialized objects of dwarf-galaxy masses in a typical galactic halo in contradiction to observation and stability of galactic discs. We present a model of double hybrid inflation which predicts density fluctuations with a small-scale cutoff to account for the ...
J. Yokoyama
semanticscholar   +7 more sources

Dwarf galaxy rotation curves and the core problem of dark matter haloes [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 2001
33 pages, 24 figures. Accepted for publication in MNRAS.
Rob A. Swaters   +2 more
semanticscholar   +7 more sources

The mass of dwarf spheroidal galaxies and the missing satellite problem [PDF]

open access: bronzeProceedings of the International Astronomical Union, 2005
4 pages, 1 figure, to appear in the proceedings of the IAUC198 "Near-Field Cosmology with Dwarf Elliptical Galaxies", H. Jerjen & B. Binggeli (eds.).
N. Wyn Evans   +4 more
arxiv   +6 more sources

Embedding globular clusters in dark matter minihaloes solves the cusp–core and timing problems in the Fornax dwarf galaxy [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT We use a fully GPU N-body code to demonstrate that dark matter (DM) minihaloes, as a new component of globular clusters (GCs), resolve both the timing and cusp–core problems in Fornax if the (five or six) GCs were recently accreted (≤3 Gyr ago) by Fornax.
Pierre Boldrini   +4 more
semanticscholar   +8 more sources

A too-many-dwarf-galaxy-satellites problem in the M 83 group [PDF]

open access: greenAstronomy & Astrophysics
Dwarf galaxies in groups of galaxies provide excellent test cases for models of structure formation. This led to a so-called small-scale crisis, including the famous missing-satellites and too-big-to-fail problems. It was suggested that these two problems can be resolved by introducing baryonic physics to cosmological simulations.
Oliver Müller   +6 more
semanticscholar   +9 more sources

Resolving the timing problem of the globular clusters orbiting the Fornax dwarf galaxy [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 2009
8 pages, 10 figures, 1 table, MNRAS in ...
Antonaldo Diaferio   +3 more
semanticscholar   +6 more sources

The Cusp/Core Problem in Galactic Halos: Long-Slit Spectra for a Large Dwarf Galaxy Sample [PDF]

open access: bronzeThe Astronomical Journal, 2005
17 pages, 14 figures; uses emulateapj. Accepted for publication in AJ.
Riccardo Giovanelli   +4 more
semanticscholar   +6 more sources

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

open access: bronzeMonthly Notices of the Royal Astronomical Society, 2016
12 pages, 14 figures, 4 tables, in press in the ...
ARCA SEDDA, MANUEL   +1 more
semanticscholar   +7 more sources

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