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[PDF] Top 20 Kitzbichler, Manfred G. (2008): Galaxy formation and evolution in the Millennium Simulation. Dissertation, LMU München: Fakultät für Physik

Has 10000 "Kitzbichler, Manfred G. (2008): Galaxy formation and evolution in the Millennium Simulation. Dissertation, LMU München: Fakultät für Physik" found on our website. Below are the top 20 most common "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

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

... of galaxy formation and evolution in the ...Croton, G. de Lucia, V. Springel, and S.D.M. White, I made use of the Millennium simulation, a very large N-body simulation of ... See full document

153

Wang, Jie
  

(2008):


	Simulating structure formation with N-Body and semi-analytic models.


Dissertation, LMU München: Fakultät für Physik

Wang, Jie (2008): Simulating structure formation with N-Body and semi-analytic models. Dissertation, LMU München: Fakultät für Physik

... of Kitzbichler & White (2007) and show evolution with redshift of the rest-frame K-band luminosity function, and of the stellar mass function ...in Kitzbichler & White ...to galaxy ... See full document

121

Giodini, Stefania
  

(2010):


	Galaxy groups in the COSMOS survey: cosmic laboratories for galaxy evolution and feedback.


Dissertation, LMU München: Fakultät für Physik

Giodini, Stefania (2010): Galaxy groups in the COSMOS survey: cosmic laboratories for galaxy evolution and feedback. Dissertation, LMU München: Fakultät für Physik

... star formation, supernova feedback, and AGN radio–mode feedback in galaxy clusters and groups (Puchwein et ...al. 2008, Bower et al. 2008, Short & Thomas ... See full document

137

Sawala, Till
  

(2011):


	Simulations of Dwarf Galaxy Formation.


Dissertation, LMU München: Fakultät für Physik

Sawala, Till (2011): Simulations of Dwarf Galaxy Formation. Dissertation, LMU München: Fakultät für Physik

... the formation and evolution of dwarf galaxies in fully cosmological, smoothed particle hydrodynamical (SPH) ...the evolution to z = 0, and because we include the environment in a consistent way, our ... See full document

172

Walch, Stefanie
  

(2008):


	The formation and early evolution of protostellar disks around low-mass stars..


Dissertation, LMU München: Fakultät für Physik

Walch, Stefanie (2008): The formation and early evolution of protostellar disks around low-mass stars.. Dissertation, LMU München: Fakultät für Physik

... the formation of very low mass objects or in case of very low initial core angular ...in galaxy formation) consider the effects of particle resolution but do not study the influence of numerical ... See full document

185

Jofré Pfeil, Paula
  

(2010):


	The age of the milky way halo stars: implications for Galaxy Formation.


Dissertation, LMU München: Fakultät für Physik

Jofré Pfeil, Paula (2010): The age of the milky way halo stars: implications for Galaxy Formation. Dissertation, LMU München: Fakultät für Physik

... Another consequence, probably more extreme, is that a significant number of stars in the Galactic halo were formed in GC’s. Although simulations of the dynamical evo- lution of globular clusters is very complicated ... See full document

165

Oser, Ludwig
  

(2012):


	Formation and evolution of massive early-type galaxies.


Dissertation, LMU München: Fakultät für Physik

Oser, Ludwig (2012): Formation and evolution of massive early-type galaxies. Dissertation, LMU München: Fakultät für Physik

... resolution galaxy formation calculations, using cosmological initial conditions, beginning to master the physics well enough to match either the winds seen in forming galaxies or the final metal distribution ... See full document

155

Hilbert, Stefan Johannes
  

(2008):


	Ray-Tracing through the Millennium Simulation.


Dissertation, LMU München: Fakultät für Physik

Hilbert, Stefan Johannes (2008): Ray-Tracing through the Millennium Simulation. Dissertation, LMU München: Fakultät für Physik

... the Millennium Simulation, the largest simulation of cosmic structure formation ever carried ...the simulation and of the lensing planes that we construct from ... See full document

103

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, ... See full document

141

Bonoli, Silvia
  

(2010):


	The Role of Galaxy Mergers in the Evolution of Supermassive Black Holes.


Dissertation, LMU München: Fakultät für Physik

Bonoli, Silvia (2010): The Role of Galaxy Mergers in the Evolution of Supermassive Black Holes. Dissertation, LMU München: Fakultät für Physik

... cosmological evolution of dark matter structures and their embedded galaxies and black ...and evolution of massive black holes, from the time when the first stars were formed to the Universe we see ...host ... See full document

147

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 in a ΛCDM universe it is necessary to carry out ...reliable simulation of the coupled nonlinear evolution of dark matter and diffuse gas, at least on the scales which determine ... See full document

158

Figueiro Spinelli, Patricia
  

(2011):


	Weak Lensing Analysis of Galaxy Groups.


Dissertation, LMU München: Fakultät für Physik

Figueiro Spinelli, Patricia (2011): Weak Lensing Analysis of Galaxy Groups. Dissertation, LMU München: Fakultät für Physik

... study galaxy associations such as clusters and ...of galaxy groups are very relevant in the field of ...to galaxy clusters, groups can be found in abundance at the redshift range where one can ... See full document

131

Suhada, Robert
  

(2011):


	The XMM-BCS galaxy cluster survey.


Dissertation, LMU München: Fakultät für Physik

Suhada, Robert (2011): The XMM-BCS galaxy cluster survey. Dissertation, LMU München: Fakultät für Physik

... the g and r band around z ≈ ...individual galaxy. An example of the galaxy density distribution in the redshift space for cluster ID 018 is shown in ... See full document

207

Franzl, Thomas
  

(2008):


	Energietransfer in Nanokristall-Kaskadenstrukturen.


Dissertation, LMU München: Fakultät für Physik

Franzl, Thomas (2008): Energietransfer in Nanokristall-Kaskadenstrukturen. Dissertation, LMU München: Fakultät für Physik

... Energie für optische Übergänge leicht manipuliert werden kann, sind sie vom UV- Bereich bis hin zu den üblichen Telekommunikationswellenlängen im nahen Infrarotbe- reich einsetzbar [46, ...Nanokristalle für ... See full document

132

Möller, Lutz
  

(2004):


	Noncommutative gauge theory and the kappa-deformed spacetime.


Dissertation, LMU München: Fakultät für Physik

Möller, Lutz (2004): Noncommutative gauge theory and the kappa-deformed spacetime. Dissertation, LMU München: Fakultät für Physik

... MPI für Plasmaphysik, Garching Aug. 1997 + Sep. 1998 Werkstudent am MPI für Quantenoptik, Garching ...Sektion Physik der LMU München Mai 1999 - ...Consulting, München Mai 2000 - ... See full document

149

Puchner, Elias M.
  

(2008):


	Einzelmolekül-Mechanoenzymatik.


Dissertation, LMU München: Fakultät für Physik

Puchner, Elias M. (2008): Einzelmolekül-Mechanoenzymatik. Dissertation, LMU München: Fakultät für Physik

... M-605, Physik Instrumente, Karlsruhe, Germany) which focuses the fluorescence light from the sample on the chip of the EMCCD camera (Andor iXon DU-888, Andor Technology, Belfast, Ireland) ... See full document

164

Buersgens, Federico
  

(2008):


	Terahertz-Nahfeldmikroskopie an Ladungsträgern in GaAs.


Dissertation, LMU München: Fakultät für Physik

Buersgens, Federico (2008): Terahertz-Nahfeldmikroskopie an Ladungsträgern in GaAs. Dissertation, LMU München: Fakultät für Physik

... Zur Erzielung von wesentlich höheren Auflösungen als die halbe Wellenlänge der verwendeten Strahlung können ultrafeine Aperturen (d.h. mit Durchmesser sehr viel kleiner als die Wellenlänge) verwendet werden, die über die ... See full document

143

Mana, Annalisa
  

(2013):


	Optically selected galaxy clusters as a cosmological probe.


Dissertation, LMU München: Fakultät für Physik

Mana, Annalisa (2013): Optically selected galaxy clusters as a cosmological probe. Dissertation, LMU München: Fakultät für Physik

... of galaxy clusters built by George Abell (Abell 1958) using the Palomar Observatory Sky Survey, then extended to include more than 4000 objects (ACO, Abell et ...peaked galaxy distribution, and nearby ... See full document

162

Steiger, Silke
  

(2008):


	Evolution of avian olfaction.


Dissertation, LMU München: Fakultät für Biologie

Steiger, Silke (2008): Evolution of avian olfaction. Dissertation, LMU München: Fakultät für Biologie

... In situ hybridization (FISH) and database mining approaches demonstrated that OR genes occur in clusters in vertebrate genomes. For example, in the human genome, 95 OR genomic clusters (6-138 genes each) could be ... See full document

139

Nastasi, Alessandro
  

(2012):


	Multiwavelength Study of high redshift galaxy clusters.


Dissertation, LMU München: Fakultät für Physik

Nastasi, Alessandro (2012): Multiwavelength Study of high redshift galaxy clusters. Dissertation, LMU München: Fakultät für Physik

... shape galaxy evolution can be studied in great ...of galaxy clus- ters at high redshift (z > 0.8) to trace the evolution of the cluster population and its matter components back to the ... See full document

155

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