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Paper: Integrated Stellar Populations of Bulges: A Midterm Report
Volume: 230, Galaxy Disks and Disk Galaxies
Page: 367
Authors: Trager, S. C.; Dalcanton, J. J.
Abstract: We are investigating the hypotheses that bulges of early-type spirals are akin to (and may in fact originally have been) intermediate-luminosity ellipticals while bulges of late-type spirals are formed from dynamical instabilities in their disks. This report discusses the current status of our on-going survey of the stellar populations of the bulges and inner disks of spirals at various points along the Hubble sequence. Absorption-line spectroscopy of the central regions of Sa-Sd spirals will be combined with stellar population models to determine integrated mean ages and metallicities.
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