Galaxy formation in the Planck cosmology – I. Matching the observed evolution of star formation rates, colours and stellar masses [PDF]
, 2014 We have updated the Munich galaxy formation model to the Planck first-year cosmology, while modifying the treatment of baryonic processes to reproduce recent data on the abundance and passive fractions of galaxies from z = 3 down to z = 0. Matching these
B. Henriques +7 more
semanticscholar +1 more source
Chemodynamical Modelling of Galaxy Formation and Evolution [PDF]
, 2002 We present our recently developed 3-dimensional chemodynamical code for galaxy evolution. This code follows the evolution of different galactic components like stars, dark matter and different components of the interstellar medium (ISM), i.e. a diffuse gaseous phase and the molecular clouds.
Rainer Spurzem +3 more
openaire +4 more sources
Galaxy formation and evolution
, 2014 How the diverse array of galaxies that are now observed originated and evolved into their present fo…
J. Silk, S. Khochfar
semanticscholar +1 more source
Galaxy formation with radiative and chemical feedback [PDF]
, 2015 Here we introduce GAMESH, a novel pipeline which implements self-consistent radiative and chemical feedback in a computational model of galaxy formation. By combining the cosmological chemical-evolution model GAMETE with the radiative transfer code CRASH,
de Bennassuti, M. +5 more
core +3 more sources
Вісник Астрономічної школи, 2004 In this work we have simulated the evolution of disk and dwarf galaxies gravitating system, using our viscosity algorithm. We investigated changes in disk galaxy chemical abundance due to minor merger of dwarf galaxy with lower abundance of heavy ...
T. A. Shumakova, P. P. Berczik
doaj +1 more source
Evolution of dwarf galaxies in the Centaurus A group [PDF]
, 2007 We consider star formation properties of dwarf galaxies in Cen A group observed within our HST/ACS projects number 9771 and 10235. We model color-magnitude diagrams of the galaxies under consideration and measure star formation rate and metallicity dependence on time.
arxiv +1 more source
Ages and metallicities of central and satellite galaxies: implications for galaxy formation and evolution [PDF]
, 2009 Using the stellar ages and metallicities of galaxies in the Sloan Digital Sky Survey (SDSS) obtained by Gallazzi et al. and the SDSS galaxy group catalogue of Yang et al., we study how the stellar ages and metallicities of central and satellite galaxies ...
A. Pasquali +6 more
semanticscholar +1 more source
Parallelization, Special Hardware and Post-Newtonian Dynamics in Direct N - Body Simulations [PDF]
, 2008 The formation and evolution of supermassive black hole (SMBH) binaries during and after galaxy mergers is an important ingredient for our understanding of galaxy formation and evolution in a cosmological context, e.g.
A. Ahmad +34 more
core +1 more source
Stochastic 2-D Models of Galaxy Disk Evolution. The Galaxy M33
Open Astronomy, 2014 We have developed a fast numerical 2-D model of galaxy disk evolution (resolved along the galaxy radius and azimuth) by adopting a scheme of parameterized stochastic self-propagating star formation.
Mineikis T., Vansevičius V.
doaj +1 more source
The E-MOSAICS project: tracing galaxy formation and assembly with the age–metallicity distribution of globular clusters [PDF]
Monthly notices of the Royal Astronomical Society, 2019 We present 25 cosmological zoom-in simulations of Milky Way-mass galaxies in the `MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE' (E-MOSAICS) project.
J. Kruijssen +3 more
semanticscholar +1 more source