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Structural properties of dwarf ellipticals and the connection with (ordinary) elliptical galaxies

dc.contributor.authorGraham, Alister
dc.date.accessioned2015-12-13T22:52:11Z
dc.date.available2015-12-13T22:52:11Z
dc.date.issued2005
dc.date.updated2016-02-24T09:49:58Z
dc.description.abstractThis article reviews the popular reasons for the belief that dwarf elliptical galaxies and (ordinary) elliptical galaxies are distinct and separate species. They include: light-profile shape (or similarly image concentration); the magnitude-central surface brightness diagram; the magnitude-effective surface brightness diagram (or similarly the magnitude-effective radius diagram); and the Fundamental Plane. It is shown how a continuous trend between luminosity and a) light-profile shape, and b) central surface brightness (until the onest of core formation at MB ∼ -20.5 mag), results in a unification of the dwarf elliptical and (ordinary) elliptical galaxies. Neither the above four reasons, nor the luminosity function (at least in the Virgo cluster) provide evidence for a division at MB = -18 mag between the dwarf elliptical and (ordinary) elliptical galaxies. Instead, they appear to be continuous extensions of each other.
dc.identifier.isbn0521852048
dc.identifier.urihttp://hdl.handle.net/1885/81455
dc.publisherCambridge University Press
dc.relation.ispartofNear-field Cosmology with Dwarf Elliptical Galaxies
dc.relation.isversionof1st Edition
dc.subjectKeywords: Dwarf, galaxies; Elliptical and lenticular, cd, galaxies; Formation, galaxies; Fundamental parameters, galaxies; Galaxies; Luminosity function, galaxies; Structure
dc.titleStructural properties of dwarf ellipticals and the connection with (ordinary) elliptical galaxies
dc.typeBook chapter
local.bibliographicCitation.lastpage310
local.bibliographicCitation.placeofpublicationCambridge, UK
local.bibliographicCitation.startpage303
local.contributor.affiliationGraham, Alister, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidGraham, Alister, u3782099
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub9746
local.identifier.doi10.1017/S1743921305003960
local.identifier.scopusID2-s2.0-63549090961
local.type.statusPublished Version

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