The Magellanic Stream, High-velocity Clouds, and the Sculptor Group

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dc.contributor.authorPutman, Mary E
dc.contributor.authorStaveley-Smith, Lister
dc.contributor.authorFreeman, Kenneth
dc.contributor.authorGibson, Bradley K
dc.contributor.authorBarnes, David G
dc.date.accessioned2015-12-13T23:09:36Z
dc.date.available2015-12-13T23:09:36Z
dc.date.issued2003
dc.date.updated2015-12-12T08:19:51Z
dc.description.abstractThe Magellanic Stream is a 100° × 10° filament of gas that lies within the Galactic halo and contains ∼2 × 108 M⊙ of neutral hydrogen. In this paper we present data from the H I Parkes All Sky Survey (HIPASS) in the first complete survey of the en
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/87068
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Galaxies: interactions; Galaxies: Local Group; Galaxy: halo intergalactic medium; Magellanic Clouds; Radio lines: general
dc.titleThe Magellanic Stream, High-velocity Clouds, and the Sculptor Group
dc.typeJournal article
local.bibliographicCitation.lastpage194
local.bibliographicCitation.startpage170
local.contributor.affiliationPutman, Mary E, University of Michigan
local.contributor.affiliationStaveley-Smith, Lister, University of Western Australia
local.contributor.affiliationFreeman, Kenneth, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationGibson, Bradley K, University of Central Lancashire
local.contributor.affiliationBarnes, David G, University of Melbourne
local.contributor.authoruidFreeman, Kenneth, u7000399
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub16198
local.identifier.citationvolume586
local.identifier.doi10.1086/344477
local.identifier.scopusID2-s2.0-0042134624
local.type.statusPublished Version

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