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</script>handle: 20.500.14352/59917
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
Astrofísica, Spiral galaxies, 52, Astrophysics (astro-ph), 500, FOS: Physical sciences, Stellar population, Astrophysics, 520, Astronomía, Astronomía (Física), [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], Evolution of galaxies
Astrofísica, Spiral galaxies, 52, Astrophysics (astro-ph), 500, FOS: Physical sciences, Stellar population, Astrophysics, 520, Astronomía, Astronomía (Física), [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], Evolution of galaxies
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