On classical and pseudo-bulges: The nature of bulges of early-type spirals

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Abstract

Historically, galactic bulges are thought to be elliptical galaxy-like objects sitting in the middle of a generally larger disk. There are, however, more and more claims that some bulges are much more similar to disks. John Kormendy has named these pseudo-bulges. In this paper I discuss some recent integral field spectroscopy of the SAURON collaboration on a sample of 24 Sa and Sab galaxies. Using their two-dimensional maps of the stellar velocity, velocity dispersion, and absorption line strength, it is now much easier to understand the nature of nearby galactic bulges. I review several aspects of bulges, namely the surface photometry, stellar kinematics, stellar populations, the presence of interstellar matter, and their behavior in the fundamental plane of early-type galaxies.

Original languageEnglish
Title of host publicationPATHWAYS THROUGH AN ECLECTIC UNIVERSE
EditorsJH Knapen, TJ Mahoney, A Vazdekis
Place of PublicationSAN FRANCISCO
PublisherASTRONOMICAL SOC PACIFIC
Pages232-241
Number of pages10
ISBN (Print)978-1-58381-650-9
Publication statusPublished - 2008
EventConference on Pathways Through and Eclectic Universe - , Spain
Duration: 23-Apr-200727-Apr-2007

Publication series

NameASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES
PublisherASTRONOMICAL SOC PACIFIC
Volume390

Other

OtherConference on Pathways Through and Eclectic Universe
Country/TerritorySpain
Period23/04/200727/04/2007

Keywords

  • EMISSION-LINE KINEMATICS
  • TELESCOPE NICMOS OBSERVATIONS
  • STELLAR POPULATION GRADIENTS
  • INTEGRAL-FIELD ABSORPTION
  • VELOCITY DISPERSION DROPS
  • PEANUT-SHAPED BULGES
  • SAURON PROJECT
  • DISK GALAXIES
  • SECULAR EVOLUTION
  • HUBBLE-SEQUENCE

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