Ram pressure strip** in high-density environments
Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …
Environmental Effects on Late‐Type Galaxies in Nearby Clusters
A Boselli, G Gavazzi - Publications of the Astronomical Society of …, 2006 - iopscience.iop.org
The transformations that take place in late‐type galaxies in the environment of rich clusters
of galaxies at z= 0 are reviewed. From the handful of late‐type galaxies that inhabit local …
of galaxies at z= 0 are reviewed. From the handful of late‐type galaxies that inhabit local …
The physical properties of star-forming galaxies in the low-redshift Universe
We present a comprehensive study of the physical properties of∼ 105 galaxies with
measurable star formation in the Sloan Digital Sky Survey (SDSS). By comparing physical …
measurable star formation in the Sloan Digital Sky Survey (SDSS). By comparing physical …
How do galaxies get their gas?
D Kereš, N Katz, DH Weinberg… - Monthly Notices of the …, 2005 - academic.oup.com
We examine the temperature history of gas accreted by forming galaxies in smoothed
particle hydrodynamics simulations. About half of the gas follows the track expected in the …
particle hydrodynamics simulations. About half of the gas follows the track expected in the …
Califa, the calar alto legacy integral field area survey-i. survey presentation
The final product of galaxy evolution through cosmic time is the population of galaxies in the
local universe. These galaxies are also those that can be studied in most detail, thus …
local universe. These galaxies are also those that can be studied in most detail, thus …
The environmental dependence of the relations between stellar mass, structure, star formation and nuclear activity in galaxies
We use a complete sample of galaxies drawn from the Sloan Digital Sky Survey to study
how structure, star formation and nuclear activity depend on local density and on stellar …
how structure, star formation and nuclear activity depend on local density and on stellar …
Semi-empirical analysis of Sloan Digital Sky Survey galaxies–I. Spectral synthesis method
The study of stellar populations in galaxies is entering a new era with the availability of large
and high-quality data bases of both observed galactic spectra and state-of-the-art …
and high-quality data bases of both observed galactic spectra and state-of-the-art …
Nearly 5000 distant early-type galaxies in COMBO-17: a red sequence and its evolution since z~ 1
We present the rest-frame colors and luminosities of~ 25,000 m R≲ 24 galaxies in the
redshift range 0.2< z≤ 1.1 drawn from 0.78 deg 2 of the COMBO-17 survey (Classifying …
redshift range 0.2< z≤ 1.1 drawn from 0.78 deg 2 of the COMBO-17 survey (Classifying …
The Sydney-AAO multi-object integral field spectrograph
We demonstrate a novel technology that combines the power of the multi-object
spectrograph with the spatial multiplex advantage of an integral field spectrograph (IFS). The …
spectrograph with the spatial multiplex advantage of an integral field spectrograph (IFS). The …
Theoretical isochrones in several photometric systems-I. Johnson-Cousins-Glass, HST/WFPC2, HST/NICMOS, Washington, and ESO Imaging Survey filter sets
We provide tables of theoretical isochrones in several photometric systems. To this aim, the
following steps are followed:(1) first, we re-write the formalism for converting synthetic stellar …
following steps are followed:(1) first, we re-write the formalism for converting synthetic stellar …