Testing the Surface Brightness Fluctuations Method for Dwarf Elliptical Galaxies in the Centaurus A Group

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dc.contributor.authorJerjen, Helmut
dc.contributor.authorFreeman, Kenneth
dc.contributor.authorBinggeli, Bruno
dc.date.accessioned2015-12-13T23:15:55Z
dc.date.available2015-12-13T23:15:55Z
dc.date.issued2000
dc.date.updated2015-12-12T08:45:48Z
dc.description.abstractWe have obtained deep B and R-band CCD photometry for five dwarf elliptical galaxies that were previously identified on Schmidt films covering the region of the Centaurus A (Cen A) group. From a Fourier analysis of the R-band CCD images we determined the
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/89134
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Galaxies: clusters: individual (Centaurus); Galaxies: distances and redshifts; Galaxies: dwarf; Galaxies: elliptical and lenticular, cD; Galaxies: individual (AM 1339-445, AM 1343-452, ESO 219-010, ESO 269-066, ESO 384-016)
dc.titleTesting the Surface Brightness Fluctuations Method for Dwarf Elliptical Galaxies in the Centaurus A Group
dc.typeJournal article
local.bibliographicCitation.lastpage176
local.bibliographicCitation.startpage166
local.contributor.affiliationJerjen, Helmut, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationFreeman, Kenneth, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBinggeli, Bruno, Universitat Basel
local.contributor.authoruidJerjen, Helmut, u9611777
local.contributor.authoruidFreeman, Kenneth, u7000399
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationMigratedxPub19060
local.identifier.citationvolume119
local.identifier.scopusID2-s2.0-3042937553
local.type.statusPublished Version

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