Results 71 to 80 of about 2,655,258 (212)

Dark Matter at the Center and in the Halo of the Galaxy [PDF]

open access: yes, 2004
All presently known stellar-dynamical constraints on the size and mass of the supermassive compact dark object at the Galactic center are consistent with a ball of self-gravitating, nearly non-interacting, degenerate fermions with mass between 76 and 491 keV, for degeneracy factor g=2. Sterile neutrinos of 76 keV mass, which are mixed with at least one
Bilic, Neven   +2 more
openaire   +2 more sources

Closing the Gap between Observed Low-mass Galaxy H i Kinematics and Cold Dark Matter Predictions

open access: yesThe Astrophysical Journal
Testing the standard cosmological model (ΛCDM) at small scales is challenging. Galaxies that inhabit low-mass dark matter halos provide an ideal test bed for dark matter models by linking observational properties of galaxies at small scales (low mass ...
Amy Sardone   +3 more
doaj   +1 more source

Halo Properties from Observable Measures of Environment: I. Halo and Subhalo Masses

open access: yesThe Open Journal of Astrophysics, 2023
The stellar mass - halo mass relation provides a strong basis for connecting galaxies to their host dark matter halos in both simulations and observations.
Haley Bowden   +2 more
doaj   +1 more source

Mitogenomic and Ecological Perspectives on the Wide‐Ridged Indo‐Pacific Finless Porpoise Neophocaena phocaenoides: Toward Emerging Conservation Strategies

open access: yesEcology and Evolution, Volume 16, Issue 9, September 2026.
IUCN‐defined extant distribution of the Indo‐Pacific finless porpoise (Neophocaena phocaenoides), overlaid with occurrence records, global Marine Protected Areas (MPAs), and Important Marine Mammal Areas (IMMAs). ABSTRACT Prior to this study, the narrow‐ridged finless porpoise (Neophocaena asiaeorientalis) had been extensively studied across East Asia,
Manokaran Kamalakannan   +7 more
wiley   +1 more source

The Outskirt Stellar Mass of Low-redshift Massive Galaxies Is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations

open access: yesThe Astrophysical Journal
Recent observations suggest that the extended stellar halos of low-redshift massive galaxies are tightly connected to the assembly of their dark matter halos.
Shuo Xu   +6 more
doaj   +1 more source

Unveiling the Functional Role of KIF21B in Microglia Inflammatory Response

open access: yesGlia, Volume 74, Issue 9, September 2026.
Microglia express KIF21B in both sexes. KIF21B binds to microglia cytoskeleton; inflammation alters such interaction promoting a phagocytic state in females. In male microglia KIF21B modulates migration. ABSTRACT Microglia are brain immune cells that maintain homeostasis and respond to injury, changing cell morphology to drive inflammation, migration ...
Danny Ganchala   +6 more
wiley   +1 more source

The clustering of galaxies in hierarchical galaxy formation models [PDF]

open access: yes, 2010
Galaxy clustering encodes information about the values of cosmological parameters and also about the physical processes behind galaxy formation and evolution. The GALFORM semi-analytical model is the theoretical approach we used to model galaxy formation.
KIM, HAN,SIK, Kim, Han Sik
core  

The Cherenkov Radiation in the Galaxy’s Halo of Dark Matter

open access: yesInternational Journal of Astronomy and Astrophysics, 2013
The effect of light refraction in a galaxy halo of dark matter, described by profiles of Navarro-Frenk-White and Burkett, was considered. Powers of the Cherenkov radiation for the refractive indexes of gravitational fields with these profiles were calculated.
openaire   +3 more sources

CFHTLenS: co-evolution of galaxies and their dark matter haloes [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2014
18 pages, MNRAS, in ...
Hudson, M.   +18 more
openaire   +4 more sources

Baryons in Dark Matter Halos

open access: yes, 2004
The existence of Dark Matter (DM) has been known since the 30's of the last century. The first cognitions from motions of galaxies in clusters and by the kinematics of individual galaxies were followed by systematic investigations, primarily via galaxy ...
Klein U, Dettmar RJ, Salucci, Paolo
core   +1 more source

Home - About - Disclaimer - Privacy