The dwarf galaxy population in Abell 2218

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dc.contributor.authorPracy, Michael
dc.contributor.authorDe Propris, Roberto
dc.contributor.authorDriver, Simon
dc.contributor.authorCouch, Warrick
dc.contributor.authorNulsen, Paul E J
dc.date.accessioned2015-12-13T22:48:55Z
dc.date.available2015-12-13T22:48:55Z
dc.date.issued2004
dc.date.updated2015-12-11T10:31:27Z
dc.description.abstractWe present results from a deep photometric study of the rich galaxy cluster Abell 2218 (z = 0.18) based on archival Hubble Space Telescope WFPC2 F606W images. These have been used to derive the luminosity function to extremely faint limits (MF606W ≈ -13
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/80286
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Galaxies luminosity function, mass function; Galaxies: clusters: general; Galaxies: dwarf
dc.titleThe dwarf galaxy population in Abell 2218
dc.typeJournal article
local.bibliographicCitation.lastpage1144
local.bibliographicCitation.startpage1135
local.contributor.affiliationPracy, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDe Propris, Roberto, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDriver, Simon, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationCouch, Warrick, University of New South Wales
local.contributor.affiliationNulsen, Paul E J, Harvard-Smithsonian Center for Astrophysics
local.contributor.authoruidPracy, Michael, u4016224
local.contributor.authoruidDe Propris, Roberto, u4039665
local.contributor.authoruidDriver, Simon, u4041024
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub8565
local.identifier.citationvolume352
local.identifier.doi10.1111/j.1365-2966.2004.08008.x
local.identifier.scopusID2-s2.0-4344685462
local.type.statusPublished Version

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