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Local galaxies as damped Lyman-alpha absorber analogues

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dc.contributor.authorZwaan, M A
dc.contributor.authorvan der Hulst, J M
dc.contributor.authorBriggs, Franklin
dc.contributor.authorVerheijen, M A W
dc.contributor.authorRyan-Weber, E V
dc.date.accessioned2015-12-13T22:43:23Z
dc.date.available2015-12-13T22:43:23Z
dc.date.issued2005
dc.date.updated2015-12-11T10:12:04Z
dc.description.abstractWe calculate in detail the expected properties of low redshift DLAs under the assumption that they arise in the gaseous disks of galaxies like those in the z ≈ 0 population. A sample of 355 nearby galaxies were analysed, for which high quality H I 21-cm
dc.identifier.isbn0521852056
dc.identifier.urihttp://hdl.handle.net/1885/79185
dc.publisherCambridge University Press
dc.relation.ispartofProbing Galaxies through Quasar Absorption Lines (C199)
dc.relation.isversionof1 Edition
dc.titleLocal galaxies as damped Lyman-alpha absorber analogues
dc.typeBook chapter
local.bibliographicCitation.lastpage119
local.bibliographicCitation.placeofpublicationCambridge, UK
local.bibliographicCitation.startpage114
local.contributor.affiliationZwaan, M A, European Southern Observatory
local.contributor.affiliationvan der Hulst, J M, University of Groningen
local.contributor.affiliationBriggs, Franklin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationVerheijen, M A W, University of Groningen Kapteyn Astronomical Institute
local.contributor.affiliationRyan-Weber, E V, University of Cambridge
local.contributor.authoruidBriggs, Franklin, u4049161
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub7682
local.identifier.doi10.1017/S1743921305002528
local.identifier.scopusID2-s2.0-63549127565
local.type.statusPublished Version

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