Results 41 to 50 of about 116,041 (186)

Stability of disk-like galaxies--Part I: Stability via reduction [PDF]

open access: yes, 2006
We prove the existence and stability of flat steady states of the Vlasov-Poisson system, which in astrophysics are used as models of disk-like galaxies.
Firt, Roman, Rein, Gerhard
core   +1 more source

ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System [PDF]

open access: yes, 2019
Astrophysics Telescope for Large Area Spectroscopy Probe is a concept for a National Aeronautics and Space Administration probe-class space mission that will achieve ground-breaking science in the fields of galaxy evolution, cosmology, Milky Way, and the
Chary, Ranga   +4 more
core  

Simulations of stellar convection, pulsation and semiconvection [PDF]

open access: yes, 2010
We report on modelling in stellar astrophysics with the ANTARES code. First, we describe properties of turbulence in solar granulation as seen in high-resolution calculations.
Bascoul   +13 more
core   +1 more source

Galaxy clusters as astrophysical laboratories and probes of cosmology [PDF]

open access: yes, 2014
Galaxy clusters are the most recent of cosmological structures to have formed by the present time in the currently favoured hierarchical scenario of structure formation and are widely regarded as powerful probes of cosmology and galaxy formation physics alike.
openaire   +2 more sources

Astrophysically motivated bulge-disc decompositions of Sloan Digital Sky Survey galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2012
28 pages, 34 figures, MNRAS ...
J. E. Gunn, C. N. Lackner
openaire   +4 more sources

Cross-correlation of the astrophysical gravitational-wave background with galaxy clustering

open access: yesPhysical Review D, 2020
We investigate the correlation between the distribution of galaxies and the predicted gravitational-wave background of astrophysical origin. We show that the large angular scale anisotropies of this background are dominated by nearby non-linear structure, which depends on the notoriously hard to model galaxy power spectrum at small scales. In contrast,
Valeri Vardanyan   +3 more
openaire   +5 more sources

Micro-Arcsecond Radio Astrometry

open access: yes, 2013
Astrometry provides the foundation for astrophysics. Accurate positions are required for the association of sources detected at different times or wavelengths, and distances are essential to estimate the size, luminosity, mass, and ages of most objects ...
Honma, M., Reid, M. J.
core   +1 more source

Giant radio galaxies as probes of the ambient WHIM in the era of the SKA

open access: yes, 2015
The missing baryons are usually thought to reside in galaxy filaments as warm-hot intergalactic medium (WHIM). From previous studies, giant radio galaxies are usually associated with galaxy groups, which normally trace the WHIM.
Chen, Ru-Rong, Peng, Bo, Strom, Richard
core   +1 more source

Theory and laboratory astrophysics [PDF]

open access: yes
Science opportunities in the 1990's are discussed. Topics covered include the large scale structure of the universe, galaxies, stars, star formation and the interstellar medium, high energy astrophysics, and the solar system.
Alcock, Charles   +9 more
core   +1 more source

Physical modelling of galaxy clusters and Bayesian inference in astrophysics

open access: yesarXiv: Cosmology and Nongalactic Astrophysics, 2019
I compare the mass values obtained with data taken from the Arcminute Microkelvin Imager (AMI) radio interferometer system and from the Planck satellite. The former of these uses a Bayesian analysis pipeline that parameterises a cluster in terms of its physical quantities, and models the dark matter \& baryonic components of a cluster using Navarro-
openaire   +2 more sources

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