Titlebook: Environment and the Formation of Galaxies: 30 years later; Proceedings of Sympo Ignacio Ferreras,Anna Pasquali Conference proceedings 2011

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jeopardize

The Cosmic Mass Density Field Reconstruction from the SDSS Group Catalog,roduced by [Wang et al., MNRAS 394, 398 (2009)]. The method uses the mass distribution in and around dark matter structures computed from cosmological simulations to map the cosmic mass distribution. This approach enables us to make reconstructions of the density field avoiding the use of arbitrary

Carcinoma

The Void Galaxy Survey,entified voids in the SDSS redshift survey on the basis of a unique geometric technique, with no a prior selection of intrinsic properties of the void galaxies. The project intends to study in detail the gas content, star formation history and stellar content, as well as kinematics and dynamics of v

Malfunction

engrave

The Dependence of Low Redshift Galaxy Properties on Environment,, group-centric radius, and the distinction between centrals and satellites; examined galaxy properties include star formation rate, colour, AGN fraction, age, metallicity and concentration. In general, satellite galaxies diverge more markedly from their central counterparts if they reside in more m

AVOID

AVOID

The Fossil Candidate RX J1548.9+0851,ynamical friction as the driving process leads to the coalescence of individual galaxies in ordinary poor groups, leaving behind nothing more than a central, massive elliptical galaxy supposed to contain the merger history of the whole group. Due to longer merging timescales for less-massive galaxie

GROSS

The Environments of Luminous Infrared Galaxies,arks an important luminosity point among IR galaxies - the large scale density of environment around LIRGs correlates strongly with their SFR above this value at a fixed stellar mass. On the other hand there is no clear correlation between stellar mass and density at constant SFR. No matter what the

智力高

,UV–IR Luminosity Functions and Stellar Mass Functions of Galaxies in the Shapley Supercluster Core, z  = 0.048, in order to investigate how the dense environment affects the galaxy properties, such as star formation (SF) or stellar mass. We find that, while the faint-end slope of optical and NIR LFs steepens with decreasing density, no environment effect is found in the slope of the SMFs. This su

增减字母法

Component Luminosity Functions of Galaxy Pairs in the MGC,ging systems (Casteels and Patton 2011). Using mock catalogues, the effect of imposing a fixed magnitude separation (.) between galaxy pairs (to isolate major mergers) is explored and we find that imposing a . introduces a selection bias which must be corrected for when comparing with field LFs. Our