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20022009
most citedIntragroup diffuse light in compact groups of galaxies II. HCG 15, 35 and 51

72 citations · 96 across the 9 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2009

Kinematic and Structural Evolution of Field and Cluster Spiral Galaxies

Bodo L. Ziegler, Elif Kutdemir, Cristiano Da Rocha +3

To understand the processes that build up galaxies we investigate the stellar structure and gas kinematics of spiral and irregular galaxies out to redshift 1. We target 92 galaxies…

astro-ph.CO2009

Velocity fields of distant galaxies with FORS2 at the VLT

Bodo L. Ziegler, Elif Kutdemir, Cristiano Da Rocha +6

We describe a method to efficiently obtain two-dimensional velocity fields of distant, faint and small, emission-line galaxies with FORS2 at the VLT. They are examined for kinemati…

astro-ph2008★ 12 cited

Internal kinematics of spiral galaxies in distant clusters III. Velocity fields from FORS2/MXU spectroscopy

E. Kutdemir, B. L. Ziegler, R. F. Peletier +8

(Abridged) We study the impact of cluster environment on the evolution of spiral galaxies by examining their structure and kinematics. Rather than two-dimensional rotation curves,…

astro-ph2008★ 72 cited

Intragroup diffuse light in compact groups of galaxies II. HCG 15, 35 and 51

C. Da Rocha, B. L. Ziegler, C. Mendes de Oliveira

This continuing study of intragroup light in compact groups of galaxies aims to establish new constraints to models of formation and evolution of galaxy groups, specially of compac…

astro-ph2005

Intra-group Light in Hickson Compact Groups

Cristiano Da Rocha, Claudia Mendes de Oliveira, Bodo L. Ziegler

We have analyzed the intra-group light component of 3 Hickson Compact Groups (HCG 79, HCG 88 and HCG 95) with detections in two of them: HCG 79, with of the total ba…

astro-ph2005

Intra-Group Light in Hickson Compact Groups - A Wavelet Approach

Cristiano Da Rocha, Claudia Mendes de Oliveira, Bodo L. Ziegler

A diffuse component of intra-group light can be observed in compact groups of galaxies. This component is presumably due to stellar material tidally stripped from the member galaxi…