H I Studies of the Sculptor Group Galaxies. VIII. The Background Galaxies: NGC 24 and NGC 45

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dc.contributor.authorChemin, Laurent
dc.contributor.authorCarignan, C
dc.contributor.authorDrouin, Nathalie
dc.contributor.authorFreeman, Kenneth
dc.date.accessioned2015-12-07T22:30:54Z
dc.date.issued2006
dc.date.updated2015-12-07T10:10:15Z
dc.description.abstractIn order to complete our H I survey of galaxies in the Sculptor group area, Very Large Array observations of NGC 24 and NGC 45 are presented. These two galaxies of similar magnitude, MB ∼17.4, lie in the background of the Sculptor group and are low surf
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/22528
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Galaxies: fundamental parameters (masses); Galaxies: halos; Galaxies: individual (NGC 24, NGC 45); Galaxies: kinematics and dynamics; Galaxies: structure
dc.titleH I Studies of the Sculptor Group Galaxies. VIII. The Background Galaxies: NGC 24 and NGC 45
dc.typeJournal article
local.bibliographicCitation.lastpage2538
local.bibliographicCitation.startpage2527
local.contributor.affiliationChemin, Laurent, Observatoire du Mont Megantic
local.contributor.affiliationCarignan, C, University of Montreal
local.contributor.affiliationDrouin, Nathalie, University of Montreal
local.contributor.affiliationFreeman, Kenneth, College of Physical and Mathematical Sciences, ANU
local.contributor.authoremailu7000399@anu.edu.au
local.contributor.authoruidFreeman, Kenneth, u7000399
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4114753xPUB22
local.identifier.citationvolume132
local.identifier.doi10.1086/508859
local.identifier.scopusID2-s2.0-33845951634
local.identifier.uidSubmittedByu4114753
local.type.statusPublished Version

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