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 …
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 …
The reversal of the star formation-density relation in the distant universe
Aims. We study the relationship between the local environment of galaxies and their star
formation rate (SFR) in the Great Observatories Origins Deep Survey, GOODS, at. Methods …
formation rate (SFR) in the Great Observatories Origins Deep Survey, GOODS, at. Methods …
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 …
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 …
WALLABY – an SKA Pathfinder H i survey
Abstract The Widefield ASKAP L-band Legacy All-sky Blind surveY (wallaby) is a next-
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …
The MeerKAT Galaxy Cluster Legacy Survey-I. Survey Overview and Highlights
K Knowles, WD Cotton, L Rudnick, F Camilo… - Astronomy & …, 2022 - aanda.org
MeerKAT's large number (64) of 13.5 m diameter antennas, spanning 8 km with a densely
packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity …
packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity …
The SAMI Galaxy Survey: instrument specification and target selection
Abstract The SAMI Galaxy Survey will observe 3400 galaxies with the Sydney-AAO Multi-
object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope in a 3-yr survey …
object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope in a 3-yr survey …