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Galaxy Formation and Evolution

Kitzbichler, Manfred G.
  

(2008):


	Galaxy formation and evolution in the Millennium Simulation.


Dissertation, LMU München: Fakultät für Physik

Kitzbichler, Manfred G. (2008): Galaxy formation and evolution in the Millennium Simulation. Dissertation, LMU München: Fakultät für Physik

... of galaxy formation in Chapter 2, where it will be also explained how to construct realistic mock observations of the simulated ...star formation histories cannot account for the observed ...

153

Guo, Qi
  

(2009):


	Galaxy Formation and Evolution in a LCDM Universe.


Dissertation, LMU München: Fakultät für Physik

Guo, Qi (2009): Galaxy Formation and Evolution in a LCDM Universe. Dissertation, LMU München: Fakultät für Physik

... follow galaxy formation directly within the evolv- ing dark matter ...structure formation (Kauffmann et ...structure formation framework provided by a dark matter ...the formation, ...

141

Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models

Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models

... of galaxy formation model in which simple analytic prescriptions (in connection with merger trees from either cosmological simulations or extended Press-Schechter formalisms) are used to model the physical ...

15

Croton, Darren
  

(2005):


	Galaxy Formation and Evolution: The Local Galaxy Population as a Cosmological Probe.


Dissertation, LMU München: Fakultät für Physik

Croton, Darren (2005): Galaxy Formation and Evolution: The Local Galaxy Population as a Cosmological Probe. Dissertation, LMU München: Fakultät für Physik

... the galaxy population: (i) How are galaxies distributed across the billions of light years that we currently observe? (ii) How do these galaxies reflect the underlying dark matter density field? (iii) What does ...

158

Galaxy Formation and Chemical Evolution

Galaxy Formation and Chemical Evolution

... star formation rate in the present work was estimated on the basis of the prevailing total surface and gas baryonic matter density of the galaxy [4] [5] [10] ...star formation rate parameter, “υ” ...

9

Understanding Galaxy Formation and Evolution with Realistic Simulations

Understanding Galaxy Formation and Evolution with Realistic Simulations

... the galaxy, building up a steep negative metallicity gradient at high ...the galaxy gradually grows in size and the metallicity gradient flattens as the galaxy ...little evolution with ...same ...

282

The detection and X-ray evolution of galaxy groups at high redshift

The detection and X-ray evolution of galaxy groups at high redshift

... of galaxy formation and evolution to include the hot, X-ray-emitting gas phase predicted to be at the virial temperatures of haloes of galaxy mass and ...a galaxy to ...

11

Topics in Galaxy Evolution: Early Star Formation and Quenching

Topics in Galaxy Evolution: Early Star Formation and Quenching

... In this thesis, we present three projects designed to shed light on yet unanswered questions on galaxy formation and evolution. The first two concern a sample of UV- bright starburst galaxies in the ...

149

A Chemical Evolution Model for the Fornax Dwarf Spheroidal Galaxy

A Chemical Evolution Model for the Fornax Dwarf Spheroidal Galaxy

... of galaxy formation and evolution have entered a new ...individual galaxy, we can obtain valuable information on its formation and ...the formation and evolution of larger ...

6

Regulation of Star Formation Amidst Heating and Cooling in Galaxies and Galaxy Clusters

Regulation of Star Formation Amidst Heating and Cooling in Galaxies and Galaxy Clusters

... and evolution of galaxies is one of the most active research fields in ...for galaxy formation and evolution is modeled by the Λ CDM, which stands for Cold Dark Mat- ter with dark energy field ...

198

A survey for stellar relics of galaxy formation in the large Magellanic cloud

A survey for stellar relics of galaxy formation in the large Magellanic cloud

... The AMR of various populations within the LMC have been studied by several authors (e.g. Cole et al. (2005); Carrera et al. (2011); Piatti et al. (2012)). Based on the AMR derived from red giant stars in the central bar, ...

168

Exploring the cosmic evolution of habitability with galaxy merger trees

Exploring the cosmic evolution of habitability with galaxy merger trees

... averaged evolution of cosmic habitability through analytic means, and the uncertainties arising from assumptions, it is difficult to constrain the distribution of galaxy habitability or its detailed de- ...

15

The Hydrangea simulations: galaxy formation in and around massive clusters

The Hydrangea simulations: galaxy formation in and around massive clusters

... a galaxy stellar mass function (GSMF) in the field that agrees with observations ...star formation and accreting supermassive black holes ...the evolution of galaxy sizes and star ...

23

The EAGLE simulations of galaxy formation: the importance of the hydrodynamics scheme

The EAGLE simulations of galaxy formation: the importance of the hydrodynamics scheme

... the formation and evolution of stars are examples of processes that occur on scales that are too small to be simulated jointly with the large-scale ...

15

nIFTy cosmology: comparison of galaxy formation models

nIFTy cosmology: comparison of galaxy formation models

... of galaxy groups – high- lighting differences amongst models, especially for the magnitude gap distribution between first- and second-ranked group ...and galaxy mergers and found that different assumptions ...

31

Evolution of supermassive black holes : the role of galaxy mergers

Evolution of supermassive black holes : the role of galaxy mergers

... local galaxy environments) semi-analytic models (SAMs) can be ...and galaxy formation modelled within the associated merger trees ...The evolution of baryons are modelled to describe star ...

156

nIFTy cosmology: the clustering consistency of galaxy formation models

nIFTy cosmology: the clustering consistency of galaxy formation models

... tures, only central galaxies are linked to a dark matter structure. Whenever a dark matter halo becomes a substructure, its galaxies become satellites and each of them receive a merging time (com- puted from the Taffoni ...

14

Observing Galaxy Formation in the First Two Billion Years

Observing Galaxy Formation in the First Two Billion Years

... The results suggest that, for luminous LAEs, current surveys do not yet have the combined sensitivity and depth to detect any sources at z ≃ 9. Although the upper limits presented in Willis & Courbin (2005) and Cuby ...

281

The evolution of galaxy structures from a Bayesian perspective

The evolution of galaxy structures from a Bayesian perspective

... The formation of the bulge component is key when modelling galaxy ...disc galaxy when viewed side-on (Figure 1.6 is an image of the Sombrero galaxy, a spiral galaxy seen edge on with a ...

207

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