EDP Sciences
Free access
Issue
A&A
Volume 395, Number 3, December I 2002
Page(s) 753 - 759
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20021352


A&A 395, 753-759 (2002)
DOI: 10.1051/0004-6361:20021352

Spatially resolved spectroscopy of Coma cluster early-type galaxies

II. The minor axis dataset
G. Wegner1, E. M. Corsini2, R. P. Saglia3, 4, R. Bender3, 4, D. Merkl3, 5, D. Thomas3, 4, J. Thomas3 and D. Mehlert6

1  Department of Physics and Astronomy, 6127 Wilder Laboratory, Dartmouth College, Hanover, NH 03755-3528, USA
2  Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
3  Universitätssternwarte München, Scheinerstraße 1, 81679 München, Germany
4  Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, 85741 Garching, Germany
5  Max-Planck-Institut für Plasmaphysik, Boltzmannstraße 2, 85748 Garching, Germany
6  Landessternwarte Heidelberg, Königstuhl, 69117 Heidelberg, Germany

(Received 8 July 2002 / Accepted 10 September 2002 )

Abstract
We present minor axis, offset major axis and one diagonal long slit spectra for 10 E and S0 galaxies of the Coma cluster drawn from a magnitude-limited sample studied before. We derive rotation curves, velocity dispersion profiles and the H3 and H4 coefficients of the Hermite decomposition of the line of sight velocity distribution. Moreover, we derive the line index profiles of Mg, Fe and H ${\beta}$ line indices and assess their errors. The data will be used to construct dynamical models of the galaxies and study their stellar populations.


Key words: galaxies: elliptical and lenticular, cD -- galaxies: kinematics and dynamics -- galaxies: stellar content -- galaxies: abundances -- galaxies: formation

Offprint request: R. P. Saglia, saglia@usm.uni-muenchen.de

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