Internal kinematics of spiral galaxies in distant clusters - II. Observations and data analysis

@article{Jaeger2004InternalKO,
  title={Internal kinematics of spiral galaxies in distant clusters - II. Observations and data analysis},
  author={K. Jaeger and B. Ziegler and Asmus Boehm and Jochen Heidt and Claus Moellenhoff and Ulrich Hopp and Roberto H. M{\'e}ndez and S. Wagner Universitaetssternwarte Goettingen and H Germany and Landessternwarte Heidelberg and Universitaetssternwarte Muenchen and Institute for Astronomy and Honolulu and Usa},
  journal={Astronomy and Astrophysics},
  year={2004},
  volume={422},
  pages={907-913}
}
We have conducted an observing campaign with the FORS instruments at the ESO-Very Large Telescope to ex- plore the kinematical properties of spiral galaxies in distant galaxy clusters. Our main goal is to analyse transformation - and interaction processes of disk galaxies within the special environment of clusters as compared to the hierarchical evolution of galaxies in the field. Spatially resolved multi object spectra have been obtained for seven galaxy clusters at 0.3 2 h we reach an S/N > 5… Expand
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References

SHOWING 1-10 OF 25 REFERENCES
The Evolution of Early-Type Galaxies in Distant Clusters*
We present results from an optical-infrared photometric study of early-type (E+S0) galaxies in 19 galaxy clusters out to z = 0.9. The galaxy sample is selected on the basis of morphologies determinedExpand
The Star Formation Histories of Galaxies in Distant Clusters
We present a detailed analysis of the spectroscopic catalog of galaxies in 10 distant clusters from Dressler et al. We investigate the nature of the different spectral classes defined by Dressler etExpand
The Tully-Fisher relation at intermediate redshift ⋆,⋆⋆
Using the Very Large Telescope in Multi Object Spectroscopy mode, we have observed a sample of 113 field spiral galaxies in the FORS Deep Field (FDF) with redshifts in the range 0.1< z< 1.0. TheExpand
The evolution of the Tully-Fisher relation of spiral galaxies
We present the B-band Tully-Fisher relation (TFR) of 60 late-type galaxies with redshifts 0.1–1. The galaxies were selected from the FORS Deep Field with a limiting magnitude of . Spatially resolvedExpand
Analysis of Spatially Resolved Emission Lines in the Spectra of Distant Galaxies
Internal kinematics is rapidly becoming an important tool for understanding the nature and evolution of distant galaxies. However, the very low signal-to-noise ratios involved in these observationsExpand
Reconstructing the history of star formation in rich cluster cores
Our study begins by revisiting the photometric Butcher–Oemler effect using data from seven CNOC clusters at We construct the foreground/background-corrected colour–magnitude diagrams for theseExpand
The FORS Deep Field: Field selection, photometric observations and photometric catalog ,
The FORS Deep Field project is a multi-colour, multi-object spectroscopic investigation of a ∼7 � × 7 � region near the south galactic pole based mostly on observations carried out with the FORSExpand
Spectroscopy of galaxies in distant clusters. IV - A catalog of photometry and spectroscopy for galaxies in seven clusters with z in the range of 0.35 to 0.55
Photometry and spectroscopy for seven deep fields containing distant clusters of galaxies with z in the range of 0.35 to 0.55 are presented. Positions and photometric parameters, includingExpand
Evolution since Z = 0.5 of the morphology-density relation for clusters of galaxies
Using traditional morphological classifications of galaxies in 10 intermediate-redshift (z similar to 0.5) clusters observed with WFPC2 on the Hubble Space Telescope, we derive relations betweenExpand
Clusters of galaxies : probes of cosmological structure and galaxy evolution
Introduction List of participants 1. Galaxy clusters as probes of cosmology and astrophysics August E. Evrard 2. Clusters of galaxies in the Sloan Digital Sky Survey Robert C. Nichol 3. ClusteringExpand
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