evolution - galaxies
The evolution of post starburst galaxies from z=2 to 0 5
... the evolution of the populations can be ob- tained from the galaxy stellar mass ...scatter galaxies into the massive end of the mass function, as our results do not re- quire accurate number densities for ...
13
The evolution of the cold interstellar medium in galaxies following a starburst
... the evolution of dust and molecular gas properties in a sample of 11 z ∼ ...(PSB) galaxies selected to span an age sequence from ongoing starburst to 1 Gyr after the starburst ...starburst galaxies ...
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An Empirically Calibrated Model for Interpreting the Evolution of Galaxies during the Reionization Era
... star-forming galaxies at z k ...break galaxies at redshifts z ’ 5 Y ...of galaxies and the Poisson ...break galaxies in the 500 Myr between z ’ 6 and 10 can be naturally explained by the ...
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Evolution of Star forming Galaxies from z=0 7 to 1 2 with eBOSS Emission line Galaxies
... the evolution of the star-forming galaxies without assuming any redshift dependency in the model parame- ters, which may distort the high-redshift results in order to fit the low-redshift ...
17
Bulgeless galaxies in the COSMOS field:environment and star formation evolution at z
... an evolution of the SFRF with decreasing cos- mic time has been already confirmed by HiZELS out to z = ...bulge-dominated galaxies with decreasing redshift (Lang et ...
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Elliptical galaxies : structure, stellar content, and evolution
... 128 galaxies in eight rich clusters at ...luminosity evolution ∆K ≈ − ...passive evolution of a stellar population that formed at high ...luminous galaxies are evolving faster than the ...
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The evolution of post starburst galaxies from z=2 to 0 5
... the evolution of the distribution of galaxies in star-formation-rate/stellar- mass/morphology planes can only help to constrain the role of different processes in shutting down star formation in combination ...
15
The extraordinary structural evolution of massive galaxies
... as evolution in related quantities such as velocity dispersion, concentration, and surface density) has received a lot of attention; it is one of the main themes of this ...structural evolution of passive ...
105
NGC 1705 and the evolution of blue compact dwarf galaxies
... We can now sketch a picture for evolution during the BCD phase and into the inactive sequence. It is in some ways similar to the stochastic self-propagating star formation picture of dwarf galaxies of ...
204
Chemical evolution of giant molecular clouds in simulations of galaxies
... notable evolution beyond 10 Myr, even though it takes up to 100 Myr for the chemical abundances to reach steady state in their ...the evolution of GMCs in a galactic ...GMC evolution in simulations ...
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Bulges and Disks in the Nearby Universe: Applications to Evolution and Formation of Galaxies
... of galaxies has contributed substantially to the understanding of the formation and evolution of ...and evolution. In addition, the structural components of galaxies in the local Universe ...
340
The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z = 3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe
... dSF galaxies increases with cosmic time, as expected from the observed metal enrichment with cosmic ...dSF galaxies tend to become the predominant type among the star-forming population at larger stellar ...
6
Evolution of the cold gas properties of simulated post starburst galaxies
... initial evolution of the star-forming gas-to-stellar mass ratio in the simulated PSBs is fairly rapid (see ...rapid evolution and reveal the processes quenching ...
15
Simulations of the formation, evolution and clustering of galaxies and quasars
... Our semi-analytic model integrates a number of differential equations for the time evolution of the galaxies that populate each hierarchical merging tree. In brief, these equations describe radiative cool- ...
42
Chan, Chi Chung (2016): Constraining the formation and evolution of cluster galaxies at z~1.5 using sizes and colour gradients. Dissertation, LMU München: Fakultät für Physik
... an evolution on the faint end of the luminosity function of the red sequence, which indicates a significant build up of the faint end of the red sequence towards lower redshift ...no evolution in the slope ...
227
Chemical evolution of star-forming galaxies in the overdense environment
... chemical evolution of individual cluster galaxies is intimately linked with the local ICM properties of the ...in galaxies as a function of the ICM density (or cluster-centric distance), there- fore ...
146
Towards Understanding The Origin And Evolution Of Ultra-Diffuse Galaxies
... " Total stellar mass in UDGs ≈ 0.2% of total cluster stellar mass " Steep size distribution -> largest UDGs very rare.. Mass measurements: Sifón+15 Size distribution [r] ...
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Evolution of the brightest cluster galaxies: the influence of morphology, stellar mass and environment
... elliptical galaxies were responsible for the building of the BCGs’ inner (elliptical-like) stellar component, whose light profile can be well represented by a S´ersic ...these galaxies continued to ...
12
Spectroscopy of Galaxies: Evolution of Escape Fractions, Metallicity Gradients and Stellar Metallicity
... lensing galaxies is described by an elliptical power-law, with a gaussian core for the brightest central galaxies, scaled according to their ...member galaxies are identified spectroscopically and/or ...
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Evolution of starburst galaxies in the Illustris simulation
... starburst galaxies are triggered by inter- action ...starburst galaxies to determine if this could be why we witness a bimodality in post-starburst populations within observational ...starburst ...
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