Abstract
The Antlia cluster (l = 273°, b = 19°) is the third nearest galaxy cluster (d = 35 Mpc) after Virgo and Fornax. In spite of its proximity, it has been poorly investigated. Its population is dominated by early type galaxies, with dwarf ellipticals being the most abundant galaxy type [1].
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
1. H. C. Ferguson, A. Sandage: AJ 100, 1 (1990)
2. B. Dirsch, T. Richtler, D. Geisler, J. C. Forte, L. P. Bassino, W. P. Gieren: AJ 125, 1908 (2003)
3. E. Bertin, S. Arnouts: A&AS 117, 393 (1996)
4. J. S. Gallagher III, R. F. G. Wyse: PASP 106, 1225 (1994)
5. A. Gil de Paz, B. F. Madore: ApJS 156, 345 (2005)
6. D. H. Jones, W. Saunders and 22 coauthors: MNRAS 355, 747 (2004)
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2007 Springer
About this paper
Cite this paper
Castelli, A. et al. (2007). Dwarf Galaxies in the Antlia Cluster: First Results. In: Saviane, I., Ivanov, V.D., Borissova, J. (eds) Groups of Galaxies in the Nearby Universe. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-71173-5_17
Download citation
DOI: https://doi.org/10.1007/978-3-540-71173-5_17
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-71172-8
Online ISBN: 978-3-540-71173-5
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)