Tully-Fisher analysis of the multiple cluster system Abell 901/902
Context. Aims. We derive rotation curves from optical emission lines of 182 disc galaxies (96 in the cluster and 86 in the field) in the region of Abell 901/902 located at z ~ 0.165. We continue the kinematic analysis presented in a previous paper. Here,
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
|01_Bosch_Tully-Fisher_analysis_of_the_2013.pdf||702.98 kB||Adobe PDF|
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