Hostname: page-component-76fb5796d-vfjqv Total loading time: 0 Render date: 2024-04-25T17:15:43.019Z Has data issue: false hasContentIssue false
  • English
  • Français

Evolution of Dwarf Galaxies in the Centaurus A Group

Published online by Cambridge University Press:  01 June 2007

L. Makarova  and
D. Makarov
L. Makarova
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Karachai-Cherkessian Republic, Russia 369167 email: lidia@sao.ru
D. Makarov
Affiliation:
Special Astrophysical Observatory, Nizhnij Arkhyz, Karachai-Cherkessian Republic, Russia 369167 email: lidia@sao.ru
Rights & Permissions [Opens in a new window]

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 consider the star formation properties of dwarf galaxies in the Cen A group observed within our HST/ACS projects number 9771 and 10235. We model color-magnitude diagrams of the galaxies under consideration and measure star formation rate and metallicity dependence on time. We study the environmental dependence of the galaxy evolution and probable origin of the dwarf galaxies in the group.

Keywords

galaxies: dwarfgalaxies: stellar contentgalaxies: formation galaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S244: Dark Galaxies and Lost Baryons , June 2007 , pp. 326 - 330
Copyright
Copyright © International Astronomical Union 2008