Results 161 to 170 of about 612 (190)

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Resolving the hot and ionized Universe through the Sunyaev-Zeldovich effect. [PDF]

open access: yesOpen Res Eur
Di Mascolo L   +25 more
europepmc   +1 more source

Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang. [PDF]

open access: yesNature
Adamo A   +27 more
europepmc   +1 more source

Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn

open access: yes
Fujimoto S   +45 more
europepmc   +1 more source

EVOLUTION OF THE GALAXY–DARK MATTER CONNECTION AND THE ASSEMBLY OF GALAXIES IN DARK MATTER HALOS [PDF]

open access: yesAstrophysical Journal, 2012
37pages, 20 figures, major revision, data updated to SDSS DR7, main conclusions remain ...
Xiaohu Yang   +2 more
exaly   +3 more sources

The Connection Between Galaxies and Their Dark Matter Halos [PDF]

open access: yesAnnual Review of Astronomy and Astrophysics, 2018
In our modern understanding of galaxy formation, every galaxy forms within a dark matter halo. The formation and growth of galaxies over time is connected to the growth of the halos in which they form. The advent of large galaxy surveys as well as high-resolution cosmological simulations has provided a new window into the statistical relationship ...
Risa H Wechsler, Jeremy L Tinker
exaly   +3 more sources

THE SPHERICALIZATION OF DARK MATTER HALOS BY GALAXY DISKS [PDF]

open access: yesAstrophysical Journal Letters, 2010
Cosmological simulations indicate that cold dark matter (CDM) halos should be triaxial. Verifying observationally this theoretical prediction is, however, less than straightforward because the assembly of galaxies is expected to modify the halo shapes and to render them more axisymmetric.
Stelios Kazantzidis   +2 more
exaly   +4 more sources

Galaxy halos and the nature of dark matter

AIP Conference Proceedings, 1995
One of the few observational facts that we know about dark matter is that within about one tenth of the virial radius, the dark halos of some galaxies have density profiles which fall with the radius as ρ(r)∝rn, where n≊0. Any successful dark matter candidate must be able to reproduce these observations.
Ben Moore, Moore Ben
exaly   +2 more sources

Dark Matter in the Halo of the Galaxy

2002
We consider a self-gravitating noninteracting fermion gas at nonzero temperature as a model for the dark matter halo of the Galaxy. This fermion gas model is then shown to imply the existence of a supermassive compact dark object at the Galactic center.
Bilić, Neven   +2 more
openaire   +3 more sources

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