The impact of accurate distances to dwarf elliptical galaxies on cosmology

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dc.contributor.authorJerjen, Helmut
dc.date.accessioned2015-12-13T22:43:29Z
dc.date.available2015-12-13T22:43:29Z
dc.date.issued2005
dc.date.updated2016-02-24T09:49:29Z
dc.description.abstractThe Surface Brightness Fluctuation method has been shown to be a powerful distance indicator for dwarf elliptical galaxies to very low surface brightness levels. It is applicable to stellar systems that are out of reach for classical indicators requiring
dc.identifier.isbn0521852048
dc.identifier.urihttp://hdl.handle.net/1885/79227
dc.publisherCambridge University Press
dc.relation.ispartofNear-field Cosmology with Dwarf Elliptical Galaxies
dc.relation.isversionof1st Edition
dc.subjectKeywords: Galaxies: clusters: individual (Virgo)-galaxies: elliptical and lenticular-galaxies: dwarf galaxies: distances and redshifts; Galaxies: luminosity function; Mass function
dc.titleThe impact of accurate distances to dwarf elliptical galaxies on cosmology
dc.typeBook chapter
local.bibliographicCitation.lastpage330
local.bibliographicCitation.placeofpublicationCambridge, UK
local.bibliographicCitation.startpage322
local.contributor.affiliationJerjen, Helmut, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidJerjen, Helmut, u9611777
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationMigratedxPub7715
local.identifier.doi10.1017/S1743921305003996
local.identifier.scopusID2-s2.0-63549151492
local.type.statusPublished Version

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