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Stellar Populations in Bulges of Spiral Galaxies

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arxiv astro-ph/0202031 v1 pith:5OKRPLMO submitted 2002-02-01 astro-ph

classification astro-ph
keywords bulgesgalaxiesspiralstellaranalysisconducteddistributionhubble
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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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