224 citations · 364 across the 6 of their papers we have counts for
6 papers
Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
Yuxiang Qin, Alan R. Duffy, Simon J. Mutch +4
We study dwarf galaxy formation at high redshift () using a suite of high- resolution, cosmological hydrodynamic simulations and a semi-analytic model (SAM). We focus on gas…
The chemical evolution of local star forming galaxies: Radial profiles of ISM metallicity, gas mass, and stellar mass and constraints on galactic accretion and winds
Rolf-Peter Kudritzki, I-Ting Ho, Andreas Schruba +4
The radially averaged metallicity distribution of the ISM and the young stellar population of a sample of 20 disk galaxies is investigated by means of an analytical chemical evolut…
The accretion histories of brightest cluster galaxies from their stellar population gradients
Paola Oliva-Altamirano, Sarah Brough, Jimmy +6
We analyse the spatially-resolved stellar populations of 9 local () Brightest Cluster Galaxies (BCGs) observed with VIMOS in IFU mode. Our sample is composed of 7 slow-rotat…
Galaxy orbits and the intracluster gas temperature in clusters
Latchezar Benatov, Ken Rines, Priyamvada Natarajan +2
In this paper we examine how well galaxies and intra-cluster gas trace the gravitational potential of clusters. Utilizing mass profiles derived from gravitational lensing and X-ray…
Interpreting the galaxy group CG J1720-67.8 through evolutionary synthesis models
S. Temporin, U. Fritze-v. Alvensleben
This paper is part of a series devoted to a detailed analysis of the properties of the compact group CG J1720-67.8 and its member galaxies with the aim of sheding light on its evol…
The type IIn supernova 1994W: evidence for the explosive ejection of a circumstellar envelope
Nikolai N. Chugai, Sergei I. Blinnikov, Robert J. Cumming +6
We present and analyse spectra of the Type IIn supernova 1994W obtained between 18 and 203 days after explosion. During the luminous phase (first 100 d) the line profiles are compo…