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Stellar Populations in Bulges of Spiral Galaxies

P. Jablonka, J. Gorgas, P. Goudfrooij

astro-pharXiv:astro-ph/0202031

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.

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