• No results found

[PDF] Top 20 Semi analytic model predictions of the galaxy population in protoclusters

Has 10000 "Semi analytic model predictions of the galaxy population in protoclusters" found on our website. Below are the top 20 most common "Semi analytic model predictions of the galaxy population in protoclusters".

Semi analytic model predictions of the galaxy population in protoclusters

Semi analytic model predictions of the galaxy population in protoclusters

... the galaxy population is described by a semi- analytic model that is based on a modified version of that presented in De Lucia & Blaizot ...combination Model Tidal ... See full document

12

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

... formation model, small objects form first from small overdensities of the density field, and then grow by accretion and mergers, in a “hierarchical” or “bottom-up” fashion (White & Rees 1978; White & Frenk ... See full document

147

Galaxy evolution in protoclusters

Galaxy evolution in protoclusters

... investigate galaxy evolution in protoclusters using a semi-analytic model applied to the Millen- nium Simulation, scaled to a Planck ...the model reproduces the observed ... See full document

14

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 ...the predictions made by the most recent generation of semi- analytic models for galaxy ...hosting galaxy clusters, which would ... See full document

153

What are protoclusters? – Defining high redshift galaxy clusters and protoclusters

What are protoclusters? – Defining high redshift galaxy clusters and protoclusters

... of protoclusters and their relationship with high-redshift clusters using the Millennium Simulation combined with a semi-analytic ...many protoclusters do not contain a main halo that is ... See full document

12

A semi-analytic model for the co-evolution of galaxies, black holes and active galactic nuclei

A semi-analytic model for the co-evolution of galaxies, black holes and active galactic nuclei

... our model predictions for the stellar mass weighted mean stellar age of galaxies as a function of stellar mass, compared with the obser- vational estimates of Gallazzi et ...the predictions from the ... See full document

33

Repeated intermittent ulipristal acetate in the treatment of uterine fibroids: a cost-effectiveness analysis

Repeated intermittent ulipristal acetate in the treatment of uterine fibroids: a cost-effectiveness analysis

... Efficacy data for UPA were limited in time compared to the duration of the analysis, and trial-based follow-up was not as frequent as required to inform monthly disease progression parameters. Therefore, interpolation ... See full document

8

Large cage assessment of a transgenic sex ratio distortion strain on populations of an African malaria vector

Large cage assessment of a transgenic sex ratio distortion strain on populations of an African malaria vector

... from model predictions, the difference from model predictions in Trials 2 and 3, though slight, is apparent by virtue of the length of the ...to model validation and enables further ... See full document

14

Semi Endogenous R&D Growth Model with Negative Population Growth

Semi Endogenous R&D Growth Model with Negative Population Growth

... growth model in which technological progress is endogenously determined to investigate how growth rates of key variables are determined when population growth is ...of population becomes, the faster ... See full document

16

Gravitational Model of the Three Elements Theory

Gravitational Model of the Three Elements Theory

... With R MG c  2 . Now it will be postulated that this Equation (16) is correct not only for long distances but for any values of x. It will be supposed also that space is no longer filled uniformly with a constant ... See full document

10

A Semi Analytic Approach to Coupled Boundary Value Problem

A Semi Analytic Approach to Coupled Boundary Value Problem

... The present problem is considered as a coupled boundary value problem and is analyzed using a semi analytic method. A series method is used to obtain the solution and region of validity is ex- tended by ... See full document

7

Galaxy modelling through stellar population synthesis

Galaxy modelling through stellar population synthesis

... Padova model the disc scale heights are assumed and then adjusted to star counts, in Besançon model the scale heights have been computed self consistently with the galactic potential: assuming an ... See full document

7

The first Super Massive Black Holes:indications from models for future observations

The first Super Massive Black Holes:indications from models for future observations

... actions with electrons in the hot corona around the SMBH. The second mode, called radio or jet mode, occurs at low accretion rates which result from an Advection Dominated Accretion Flow (ADAF - Rees 1982) that typically ... See full document

17

A Review on health care examination records using data mining

A Review on health care examination records using data mining

... In this paper, study Overall health inspection is companion essential a part of care in several countries. Distinctive the participants in hazard are very important for early notice and preventive intervention. The ... See full document

5

The Novel Interaction Model of Dark Energy and Dark Matter

The Novel Interaction Model of Dark Energy and Dark Matter

... interaction model of Dark Matter and Dark Energy. Using the new model, the paper studies the char- acteristic property of the gravity in the very early ... See full document

6

SDSS IV MaNGA : spatially resolved star formation histories in galaxies as a function of galaxy mass and type

SDSS IV MaNGA : spatially resolved star formation histories in galaxies as a function of galaxy mass and type

... stellar population parameters such as age and chemical element ra- tios (Mehlert et ...where galaxy centres are more metal-rich, and star formation continues in the central regions, with enriched material, ... See full document

34

Multi-model ensembles improve predictions of crop-environment-management interactions

Multi-model ensembles improve predictions of crop-environment-management interactions

... target population. The target population corresponding to the AgMIP wheat pilot data set is worldwide wheat ...that population, and the prediction problem is prediction for a randomly chosen ... See full document

13

Restarted Adomian Decomposition Method for Solving Volterra’s Population Model

Restarted Adomian Decomposition Method for Solving Volterra’s Population Model

... an analytic approxima- tion for Volterra’s model for population growth of a species within a closed system, called the Restarted Adomian decomposition method (RADM) to solve the ... See full document

9

Hybrid simulation:historical lessons, present challenges and futures

Hybrid simulation:historical lessons, present challenges and futures

... DES model might well “optimize” flow within the ED itself, but cannot properly take into account these other factors without growing into a mega-model of the whole hospital and the community it ... See full document

16

Factor analytic multiplicative mixed models in the analysis of multiple experiments

Factor analytic multiplicative mixed models in the analysis of multiple experiments

... mixed model setting, Piepho (1998) presented a factor analytic multiplicative mixed (FAMM) model with random genotype and g x e effects which is conceptually and functionally better than ... See full document

23

Show all 10000 documents...