A&A 383, 30-45 (2002)
DOI: 10.1051/0004-6361:20011699
New UBVRI colour distributions in E-type galaxies
I. The data ,
T. P. Idiart1, R. Michard2 and J. A. de Freitas Pacheco31 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: thais@iagusp.usp.br
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: pacheco@obs-nice.fr
(Received 17 September 2001 / Accepted 7 November 2001)
Abstract
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
U-V 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
Offprint request: R. Michard, michard@obspm.fr
SIMBAD Objects
Tables at the CDS
© ESO 2002

BibSonomy
CiteUlike
Del.icio.us
Digg
Facebook
Mendeley
Twitter