Internal kinematics of spiral galaxies in distant clusters

2008/06/28 by Elif Kutdemir, E. Kutdemir, B. Ziegler +12
Physics and Astronomy · #Astronomy and Astrophysical Research #Galaxies: Formation, Evolution, Phenomena #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809782

accepted for publication in A&A, high resolution version available at http://www.astro.rug.nl/~kutdemir/papers/

arxiv created 2008/06/28 · openalex publication_date 2008/07/01 · arxiv updated 2009/12/01 · openalex created_date 2020/01/23 · openalex updated_date 2026/07/31

Abstract

Context. We continue our investigation on how the cluster environment affects the evolution of galaxies.

Citations

• Parametric Recovery of Line-of-Sight Velocity Distributions from Absorption-Line Spectra of Galaxies via Penalized Likelihood
• Kinemetry: a generalization of photometry to the higher moments of the line-of-sight velocity distribution
• A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s