Volume 383, Number 1, FebruaryIII 2002
|Page(s)||30 - 45|
|Section||Cosmology (including clusters of galaxies)|
|Published online||15 February 2002|
I. The data
Instituto de Astronomia, Geofisica e Ciências Atmosféricas, Depto. de Astronomia, Universidade de São Paulo, Av. Miguel Stefano, 4200-CEP, 04301-904 S. Paulo, SP-Brazil e-mail: firstname.lastname@example.org
2 Observatoire de Paris, LERMA, 77 Av. Denfert-Rochereau, 75015 Paris, France e-mail: Raymond.Michard@obspm.fr
3 Observatoire de la Côte d'Azur, Département Augustin Fresnel, BP 4229, 06304 Nice Cedex 4, France e-mail: email@example.com
Corresponding author: R. Michard, firstname.lastname@example.org
Accepted: 7 November 2001
New colour distributions have been derived from wide field UBVRI frames for 36 northern bright elliptical galaxies and a few lenticulars. The classical linear representations of colours against were derived, with some improvements in the accuracy of the zero point colours and of the gradients. The radial range of significant measurements was enlarged both towards the galaxy center and towards the outskirts of each object. Thus, the “central colours”, integrated within a radius of 3´´, and the “outermost colours” averaged near the surface brightness could also be obtained. Some typical deviations of colour profiles from linearity are described. Colour-colour relations of interest are presented. Very tight correlations are found between the colour and the Mg2 line-index, measured either at the Galaxian center or at the effective radius.
Key words: galaxies: elliptical and lenticulars, CD / galaxies: ISM
© ESO, 2002
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.