Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S262(5), p. 398-399, 2009

DOI: 10.1017/s1743921310003406

Links

Tools

Export citation

Search in Google Scholar

Stellar populations of disc galaxies: from the center of the bulge to the edge of the disc

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Green circle
Postprint: archiving allowed
Red circle
Published version: archiving forbidden
Data provided by SHERPA/RoMEO

Abstract

AbstractWe present extensive photometric and spectroscopic study to give a new insight in the bulge stellar population. Super-solar α/Fe and its constant value along the radial profile, in most of the galaxies, suggest that the star formation in these objects has been fast and occurred at the same time in the whole bulge.

Beta version