Stellar Populations in Bulges of Spiral Galaxies

Abstract

We have conducted a spectroscopic analysis of the bulges of a sample of 31 spiral galaxies, spanning the Hubble sequence from S0 to Scd type, in order to study the radial distribution of their stellar population properties.

To be published in "The Evolution of Galaxies. II. Basic Building Blocks", ed. M. Sauvage et al., Kluwer

References in corpus (2)

• The Luminosity-Metallicity Relation for Bulges of Spiral Galaxies
• Line-Strength Indices in Bright Spheroidals: Evidence for a Stellar Population Dichotomy between Spheroidal and Elliptical Galaxies

Cited by in corpus (4)

• Morphologies and stellar populations of galaxies in the core of Abell 2218
• Secular Evolution of Spiral Galaxies
• Stellar Population Gradients in Bulges along the Hubble Sequence: I. The Data
• Galaxy Secular Mass Flow Rate Determination Using the Potential-Density Phase Shift Approach: Application to Six Nearby Spiral Galaxies