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Issue Astron. Astrophys. Suppl. Ser.
Volume 128, Number 1, February_II 1998
Page(s) 75 - 109
DOI http://dx.doi.org/10.1051/aas:1998378

DOI: 10.1051/aas:1998378

A&A Supplement series, Vol. 128, February II 1998, 75-109

Received March 11; accepted June 16, 1997

Extended ionized gas in elliptical galaxies

II. Velocity and monochromatic maps of 11 elliptical and lenticular galaxiesgif

H. Plana tex2html_wrap514, J. Boulesteix tex2html_wrap516, Ph. Amram tex2html_wrap516, C. Carignan tex2html_wrap520, and C. Mendes de Oliveira tex2html_wrap522

Send offprint request: H. Plana

tex2html_wrap524  Observatoire de Marseille, 2 Place Le Verrier, F-13248 Marseille Cedex 04, France

tex2html_wrap526  Instituto Astronômico e Geofísico (IAG), Av. Miguel Stefano 4200 CEP: 04301-904 São Paulo, Brazil

tex2html_wrap528  Dept. de Physique, Université de Montréal CP 6128, Succ. Centre ville Montréal, P.GC Canada, H3C-3J7, Canada

Abstract:

For the last ten years faint ionized gas detection has been carried out for elliptical galaxies with success. The kinematics is essential to understand galaxy gas origin and fate. Here we present a sample of 11 elliptical and lenticular galaxies observed with the "Cigale" scanning Perot-Fabry instrument. For each galaxy monochromatic and velocity map of ionized gas is presented. Geometrical properties such as viewing angles and axis ratios are also derived from observations. Double gaseous components are found in 3 galaxies of our sample, implying an external origin for at least part of the observed gas.

keywords: galaxies: elliptical and lenticular, kinematics, ISM

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Copyright by the European Southern Observatory (ESO)



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