Abstract
The stellar populations in the bulges of S0s, together with the galaxies' dynamics, masses and globular clusters, contain very interesting clues about their formation. I present here recent evidence suggesting that S0s are the descendants of fading spirals whose star formation ceased. © 2008 Copyright International Astronomical Union 2008.
Author supplied keywords
Cite
CITATION STYLE
APA
Aragón-Salamanca, A. (2007). Stellar populations in the bulges of S0s and the formation of S0 galaxies. In Proceedings of the International Astronomical Union (Vol. 3, pp. 285–288). Cambridge University Press. https://doi.org/10.1017/S1743921308017924
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free