Results 141 to 150 of about 12,885 (260)
Universal relations with fermionic dark matter
We have recently introduced a new model for the distribution of dark matter (DM) in galaxies, the Ruffini-Argüelles-Rueda (RAR) model, based on a self-gravitating system of massive fermions at finite temperatures.
Krut A. +3 more
doaj +1 more source
[ITAL]Hubble[/ITAL] [ITAL]Space[/ITAL] [ITAL]Telescope[/ITAL] Observations of the Draco Dwarf Spheroidal Galaxy [PDF]
Carl J. Grillmair +17 more
openalex +1 more source
A [ITAL]V[/ITAL] and [ITAL]I[/ITAL] CCD Mosaic Survey of the Ursa Minor Dwarf Spheroidal Galaxy [PDF]
Jan Kleyna +4 more
openalex +1 more source
Tidal Disruption and Tails from the Carina Dwarf Spheroidal Galaxy [PDF]
J. R. Kuhn +2 more
openalex +1 more source
WFPC2 Observations of the Ursa Minor Dwarf Spheroidal Galaxy [PDF]
Kenneth J. Mighell, Christopher J. Burke
openalex +1 more source
Searching for very-high-energy photons arising from dark matter interactions in selected astrophysical environments is a promising strategy to probe the existence and particle nature of dark matter.
Mani Khurana +4 more
doaj +1 more source
Supernova-driven outflows and chemical evolution of dwarf spheroidal galaxies. [PDF]
Qian YZ, Wasserburg GJ.
europepmc +1 more source
Upper limits to the H I content of the dwarf spheroidal galaxies
G. R. Knapp, F. J. Kerr, P. F. Bowers
openalex +1 more source
The globular cluster system of the Sagittarius dwarf spheroidal galaxy: the age of Terzan 8 [PDF]
Montegriffo +5 more
openalex +1 more source
Low-mass quiescent galaxies are thought to predominantly reside in overdense regions, as environmental effects are often invoked to explain their shutdown of star formation. These longer-timescale quenching mechanisms—such as interactions with hot gas in
Sam E. Cutler +23 more
doaj +1 more source

