Bibcode
Falcón-Barroso, J.; Bacon, R.; Bureau, M.; Cappellari, M.; Davies, R. L.; de Zeeuw, P. T.; Emsellem, E.; Fathi, K.; Krajnović, D.; Kuntschner, H.; McDermid, R. M.; Peletier, R. F.; Sarzi, M.
Referencia bibliográfica
Science Perspectives for 3D Spectroscopy, Eso Astrophysics Symposia European Southern Observatory. ISBN 978-3-540-73490-1. Springer-Verlag Berlin Heidelberg, 2007, p. 111
Fecha de publicación:
0
2007
Número de citas
2
Número de citas referidas
2
Descripción
We present results from our ongoing effort to understand the nature and
evolution of nearby galaxies using the SAURON integral-field
spectrograph. In this proceeding we focus on the study of the particular
case formed by the interacting galaxies NGC5953 and NGC5954. We present
stellar and gas kinematics of the central regions of NGC5953. We use a
simple procedure to determine the age of the stellar populations in the
central regions and argue that we may be witnessing the formation of a
kinematically decoupled component (hereafter KDC) from cold gas being
acquired during the ongoing interaction with NGC5954.