Hostname: page-component-cc8bf7c57-l9twb Total loading time: 0 Render date: 2024-12-12T07:35:24.371Z Has data issue: false hasContentIssue false
  • English
  • Français

On the Nature of Dwarf Galaxies in the Interacting Group HCG 31

Published online by Cambridge University Press:  26 May 2016

Ángel R. López-Sánchez ,
César Esteban  and
Mónica Rodríguez
Ángel R. López-Sánchez
Affiliation:
Instituto de Astrofísica de Canarias, E38200, Tenerife, Spain
César Esteban
Affiliation:
Instituto de Astrofísica de Canarias, E38200, Tenerife, Spain
Mónica Rodríguez
Affiliation:
INAOE, Apdo. Postal 51 y 216, 72000 Puebla, Pue., México

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have analysed the morphology, kinematics, colors and chemical composition of the ionized gas of the different objects belonging to the interacting compact group HCG 31 in order to get a global view of the origin and evolution of the dwarf galaxies present in it.

Type
Part 4. Recycling
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 568 - 569
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

López-Sánchez, A.R. & Esteban, C. 2003, in Satellites and tidal streams, Prada, F. and Martínez-Delgado, D. (eds), in prep.Google Scholar
Williams, B.A., McMahon, P.M. & van Gorkom, J.H. 1991, AJ, 101, 1957.CrossRefGoogle Scholar