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What Can We Learn From Dynamics Of Nearby Galaxies To Study Distant Galaxies?

Published online by Cambridge University Press:  01 August 2006

B. Epinat ,
P. Amram  and
C. Balkowski
B. Epinat
Affiliation:
Laboratoire d'Astrophysique de Marseille, Observatoire Astronomique Marseille-Provence, 2 place Le Verrier, 13248 Marseille Cedex 04, France – email: [email protected]
P. Amram
Affiliation:
Laboratoire d'Astrophysique de Marseille, Observatoire Astronomique Marseille-Provence, 2 place Le Verrier, 13248 Marseille Cedex 04, France – email: [email protected]
C. Balkowski
Affiliation:
Laboratoire Galaxies Etoiles Physique et Instrumentation, Observatoire de Paris-Meudon, 5 place Jules Janssen, 92195 Meudon Cedex, France
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This is an ongoing project.

During last few years, new instruments like GIRAFFE (Flores, H., Hammer, F., Puech, M., et al., 2006, A&A 455,107) or SINFONI (Förster Schreiber, N.M., Genzel, R., Lehnert, M.D., et al., 2006, ApJ 645,1062) have began investigations on 3D kinematics of high redshift galaxies. This is just the head of the iceberg as Extremely Large Telescope will allow this kind of study on a larger sample. By now, it is important to be able to recover the actual kinematic parameters, and overall to disentangle evolutionnary effects from distance effects.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 401
Copyright
Copyright © International Astronomical Union 2007