Cl 1358+62: Characterizing the Physical Properties of Cluster Galaxies atz= 0.33

2003/02/14 by Kim-Vy Tran, Kim‐Vy Tran, Luc Simard +3 · 25 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Cluster (spacecraft) #Computer network #Computer science #Galaxy #Galaxy cluster #Physics #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1086/374831

published in The Astrophysical Journal 590(1), 238-255 (IOP Publishing) · Accepted by ApJ; includes extensive discussion on reliability of fitting 2D bulge/disk models. Higher resolution images available at http://www.exp-astro.phys.ethz.ch/vy/astronomy/cl1358.ps.gz

arxiv created 2003/02/14 · openalex publication_date 2003/06/10 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Peer reviewed: Yes

Citations

• The Evolution of Balmer Absorption-Line Strengths in E/S0 Galaxies from [FORMULA][F]z=0[/F][/FORMULA] to [FORMULA][F]z=0.83[/F][/FORMULA]
• The Evolution of Early‐Type Galaxies in Distant Clusters. III. \documentclassaastex \usepackageamsbsy \usepackageamsfonts \usepackageamssymb \usepackagebm \usepackagemathrsfs \usepackagepifont \usepackagestmaryrd \usepackagetextcomp \usepackageportland,xspace \usepackageamsmath,amsxtra \usepackage[OT2,OT1]fontenc \newcommand\cyr \renewcommand\rmdefaultwncyr \renewcommand\sfdefaultwncyss \renewcommand\encodingdefaultOT2 \normalfont \selectfont \DeclareTextFontCommand\textcyr\cyr \pagestyleempty \DeclareMathSizes10976 \begindocument \landscape M/ L_V \enddocument Ratios in the \documentclassaastex \usepackageamsbsy \usepackageamsfonts \usepackageamssymb \usepackagebm \usepackagemathrsfs \usepackagepifont \usepackagestmaryrd \usepackagetextcomp \usepackageportland,xspace \usepackageamsmath,amsxtra \usepackage[OT2,OT1]fontenc \newcommand\cyr \renewcommand\rmdefaultwncyr \renewcommand\sfdefaultwncyss \renewcommand\encodingdefaultOT2 \normalfont \selectfont \DeclareTextFontCommand\textcyr\cyr \pagestyleempty \DeclareMathSizes10976 \begindocument \landscape z=0.33 \enddocument Cluster Cl 1358+62
• Quantitative Morphology of the Intermediate-Redshift Galaxy Cluster Abell 2443 from Ground-based Imaging: Evidence for a Galaxy Concentration Index Correlation with Cluster Density
• Equation of State Calculations by Fast Computing Machines
• A High Merger Fraction in the Rich Cluster MS 1054−03 at [CLC][ITAL]z[/ITAL][/CLC] = 0.83: Direct Evidence for Hierarchical Formation of Massive Galaxies
• The Asymmetry of Galaxies: Physical Morphology for Nearby and High‐Redshift Galaxies
• The Color‐Magnitude Relation in CL 1358+62 atz= 0.33: Evidence for Significant Evolution in the S0 Population
• Extragalactic nebulae.

Cited by

• Field E+A Galaxies at Intermediate Redshifts (0.3 <z< 1)
• Identifying Lenses with Small‐Scale Structure. II. Fold Lenses
• ZFIRE: Measuring Electron Density with [O ii] as a Function of Environment at z = 1.62