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2.14. Stellar and ionized gas-velocity fields in the central regions of a sample of galaxies

Published online by Cambridge University Press:  25 May 2016

C. del Burgo ,
S. Arribas ,
E. Mediavilla  and
B. García-Lorenzo
C. del Burgo
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Canary Islands, Spain
S. Arribas
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Canary Islands, Spain
E. Mediavilla
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Canary Islands, Spain
B. García-Lorenzo
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Canary Islands, Spain

Abstract

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We present the velocity fields for the ionized gas and the stars obtained from 2D fibre spectroscopy in the central regions of a sample of active (NGC 985, NGC 1052, NGC 6500) and non-active (M31, M32) galaxies.

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 85 - 86
Copyright
Copyright © Kluwer 1998 

References

García, A., Rasilla, J. L., Arribas, S., and Mediavilla, E. (1994): Instrumentation in Astronomy, Vol 2198, ed. Crawford, D. L. and Craine, C. R. (Hawaii: SPIE), 75.CrossRefGoogle Scholar
García-Lorenzo, B., Mediavilla, E., Arribas, S. & del Burgo, C. (1997): ApJL, 483, 99.Google Scholar