Scaling Relations of Field Spirals at intermediate Redshift

Details Scaling Relations of Field Spirals at intermediate Redshift Scaling Relations of Field Spirals at intermediate Redshift

2002-10-15

arxiv.org/abs/astro-ph/0210317v2

Astrophys.Space Sci. 284 (2003) 689-692

Astronomy and Astrophysics

Astrophysics

4 pages, 2 eps-figures, to appear in "The Evolution of Galaxies III. From Simple Approaches to Self-Consistent Models", procee

Scientific paper

10.1023/A:1024047115089

In the last few years, galaxies at redshifts up to z~1 have become accessible for medium-resolved spectroscopy thanks to the new generation of 10m-class telescopes. With kinematic and photometric information on spiral galaxies in this regime, well-known scaling relations like the Tully-Fisher relation (TFR) can be studied over half a Hubble time. By comparison to local samples, these studies facilitate simultaneous tests of the hierarchical merging scenario and stellar population models. Using the Very Large Telescope, we obtained spatially resolved rotation curves of 78 spiral galaxies in the FORS Deep Field (FDF), covering all Hubble types from Sa to Sm/Irr at redshifts 0.1

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