搜索结果: 1-14 共查到“星系形成与演化 galaxies”相关记录14条 . 查询时间(0.357 秒)
Sky survey reveals newborn jets in distant galaxies（图）
Sky survey newborn jets distant galaxies
font style='font-size:12px;'>
2020/12/11
Astronomers using data from the ongoing VLA Sky Survey have found distant galaxies with supermassive black holes at their cores that have launched powerful, radio-emitting jets of material w...
Growth of galaxies in SPH simulations
Explore Galaxy formation. Smooth particle hydrodynamics The universe simulation Galactic gas Temperature history Galaxy star
font style='font-size:12px;'>
2014/12/9
We explore the growth of galaxies formed in self-consistent Smoothed Particle Hydrodynamic (SPH) cosmological simulations. In the first Chapter, we examine the temperature history of gas accreted by f...
Evolution in the clustering strength of radio galaxies
galaxies active Galaxies galaxies evolution Galaxies
font style='font-size:12px;'>
2011/10/20
We cross match the NVSS and FIRST surveys with three large photometric catalogues of luminous red galaxies (LRGs) to define radio-loud samples. These have median redshifts 0.35, 0.55 and 0.68 and, by ...
Galaxy Zoo: Dust lane early-type galaxies are tracers of recent, gas-rich minor mergers
galaxies: evolution — galaxies: interactions — galaxies: active — galax-ies: elliptical and lenticular
font style='font-size:12px;'>
2011/10/17
We present the second of two papers concerning the origin and evolution of local early-type galaxies exhibiting dust features. We use optical and radio data to examine the nature of AGN activity in th...
The ATLAS3D Project-- VIII: Modelling the Formation and Evolution of Fast and Slow Rotator Early-Type Galaxies within $Λ$CDM
galaxies elliptical and lenticular cD – galaxies formation – galaxies evolution – galaxies structure
font style='font-size:12px;'>
2011/10/21
We propose a simple model for the origin of fast and slow rotator early-type galaxies (ETG) within the hierarchical $\Lambda$CDM scenario, that is based on the assumption that the mass fraction of ste...
The evolution of galaxies in compact and fossil groups
evolution of galaxies compact fossil groups
font style='font-size:12px;'>
2009/6/26
The evolution of galaxies in compact and fossil groups。
AGN Activity and Circumnuclear Star Formation in Nearby Galaxies
Circumnuclear Star Formation Nearby Galaxies
font style='font-size:12px;'>
2009/6/18
AGN Activity and Circumnuclear Star Formation in Nearby Galaxies。
The chemical evolution of gas-rich dwarf galaxies
chemical evolution gas-rich dwarf galaxies
font style='font-size:12px;'>
2009/6/11
The chemical evolution of gas-rich dwarf galaxies。
Dynamical Evolution of Clusters of Galaxies
Dynamical Evolution Clusters of Galaxies
font style='font-size:12px;'>
2009/6/11
Dynamical Evolution of Clusters of Galaxies。
The evolution of disk galaxies
disk galaxies evolution
font style='font-size:12px;'>
2009/6/8
The evolution of disk galaxies。
Properties of Disk Galaxies in a Hierarchical Formation Scenario
Galaxies evolution fundamental parameters cosmologyl darak matter
font style='font-size:12px;'>
2009/6/4
Properties of Disk Galaxies in a Hierarchical Formation Scenario。
THE FUTURE OF GALAXIES AND THE FATE OF INTELLIGENT LIFE
GALAXIES gaseous content INTELLIGENT LIFE
font style='font-size:12px;'>
2009/3/19
We investigate the influence of recent advances in research on the
gaseous content of the universe on our knowledge of star formation histories of spiral
galaxies. The discovery of low-redshift popu...
The Fate of Dwarf Galaxies in Clusters and the Origin of Intracluster Stars
Cosmology—galaxies clusters dwarfs interactions—methods numerical
font style='font-size:12px;'>
2010/9/15
The main goal of this paper is to compare the relative importance of destruction by tides vs. destruction by mergers, in order to assess if tidal destruction of galaxies in clusters is a viable scenar...
WHY THERE ARE NO ELLIPTICAL GALAXIES MORE FLATTENED THAN E7. THIRTY YEARS LATER
dark matter-Galaxies evolution-Galaxies formation-Galaxies halos-Galaxies structure
font style='font-size:12px;'>
2009/2/18
WHY THERE ARE NO ELLIPTICAL GALAXIES MORE FLATTENED THAN E7. THIRTY YEARS LATER。