Color-Magnitude diagram for Perseus galaxies with Local. Group dEs plotted. Cluster dEs deviate from the color-magnitude relation. Conselice, Gallagher & Wyse (2003) ...
... Davies, Erwin de Blok, Virginia Kilborn, Suzanne Linder, Karen Masters, Martin ... Low column-density gas in the local Universe. Extragalactic OH Megamaser ...
First Results from an HST/ACS Snapshot Survey of Intermediate Redshift, Intermediate X-ray Luminosity Clusters of Galaxies: Early Type Galaxies and Weak Lensing
Tully-Fisher relation of high-z spirals (with Osamu Nakamura, Bo Milvang-Jensen ... Tully-Fisher relation of low-z S0s (with Alejandro Garcia-Bedregal and Mike ...
Find 3:1 ratio, flat or increasing with redshift. HST ACS color image ... Treister & Urry 2006: meta-analysis shows obs/unobs ratio flat or increases with z ...
Red galaxies are the ones with bulges. DEEP 1 galaxies with HST imaging (fits by L. Simard) ... brighter bulges. COMBO- 17 photometric survey. Large area, 17 ...
During the mid-90's, with improved instrumentation, the commissioning of the 8-m ... VLA, ultra deep HDF-N ( Merlin, WSRT) JCMT SCUBA sub-mm maps of HDF-N ...
Anomalous Cosmic Rays (ACR) Radio emissions. Inferred complications. Inner/Outer heliosheaths ... No evidence of local generation of Anomalous Cosmic Rays (ACRs) ...
First Year Physics First Year organisers: - Dr Sue Francis (MR13) (susan.francis@nottingham.ac.uk) - Dr Anne Green (CAPT) (anne.green@nottingham.ac.uk)
35% of bulge-dominated galaxies experienced a merger with mass ratio 1:4 in the ... For both field and cluster galaxies, the merger events are dominated by Sp-Sp ...
Dark matter cusps in galaxy centers, in particular absent in ... dynamical friction and smooth any cusp. in dwarf galaxies. The material is more dissipative, ...
Apparent brightening of ~0.7 mag. BUT it can be entirely explained by ... The apparent brightening of the B band TF is entirely due to selection effects ...
... Redshift Survey, which uses the DEIMOS spectrograph on the Keck II telescope, is ... DEEP2 is similar to LCRS in sample size but at z=1 - with a very ...
From red to blue, the spectrum of visible light covers one octave in frequency. ... data handling and data analysis, and cooperation in a multi-national enterprise. ...
Fusions de galaxies fr quentes ( a N2s-3 d'apr s simulations num riques) ... Ajustement par une ou deux fonctions de Schechter ou par Schechter Gaussienne ...
1. Diffuse light. in clusters of galaxies. Florence DURRET. Institut d'astrophysique de Paris ... The example of Coma: discovery of several weak diffuse sources ...
GOYA Team: Carmen Eliche-Moral, David Crist bal, Lilian Dom nguez, ... Using upcoming EMIR NIR multi-object spectrograph on 10.2 m GTC. UFL, UCM, Toulouse, IAC ...
Resolved kinematics of galaxies (Cooper et al., in prep) The dependence of galaxy properties on environment (Cooper/Gerke/Madgwick et al., in prep) ...
and quasar winds. on the AGN population (Fontanot, Monaco, Cristiani & Tozzi 2006) ... Quasar selected with 3.5 z 5.2. Also included Ly-break and Seyfert Galaxies ...
Early Results from the DEEP2 Redshift Survey. Jeffrey Newman. and the DEEP2 Team ... relative velocities of faint neighbors of bright galaxies (ala Prada et al. 2003) ...
X-ray Astronomy in the Next Decade. 90% of the matter in the universe can only be ... M.Begelman, TJ Cox, D. Croton, T. DiMatteo, I. George, C. Martin, J. Ostriker, V. ...
We will need to investigate what types of objects we miss in more detail (mostly just mag. ... By comparing the universe at high redshift to what is seen ...
Separate POINT/AGAPE search has 5 good events: 4 on far side, 1 on near; no conclusions ... clear: need more M31 work (MEGA/POINT-AGAPE, etc); Supermacho on LMC. ...