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dc.contributor.authorBowen, D.V.
dc.contributor.authorHuchtmeier, W.
dc.contributor.authorBrinks, E.
dc.contributor.authorTripp, T.M.
dc.contributor.authorJenkins, E.B.
dc.date.accessioned2007-08-11T20:14:14Z
dc.date.available2007-08-11T20:14:14Z
dc.date.issued2001-06
dc.identifier.citationBowen , D V , Huchtmeier , W , Brinks , E , Tripp , T M & Jenkins , E B 2001 , ' 21-cm H I emission from the Damped Lyman-alpha absorber SBS 1543 593 ' , Astronomy and Astrophysics , vol. 372 , pp. 820-823 . https://doi.org/10.1051/0004-6361:20010592
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 175762
dc.identifier.otherPURE UUID: db9b9d7a-456c-439f-a504-4dfd0f0a34b0
dc.identifier.otherdspace: 2299/352
dc.identifier.otherScopus: 0035373271
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407893
dc.identifier.urihttp://hdl.handle.net/2299/352
dc.descriptionOriginal article can be found at: http://www.aanda.org/--Copyright The European Southern Observatory DOI : 10.1051/0004-6361:20010592
dc.description.abstractWe detect 21-cm emission from the Low Surface Brightness (LSB) galaxy SBS 1543+593, which gives rise to a Damped-Ly (DLy ) absorption line in the spectrum of the background QSO HS 1543+5921 (ze = 0:807). We obtain an accurate measure of the velocity of the H I gas in the LSB galaxy, v = 2868 km s−1, and derive a mass of MHI = 1:3 109 M . We compare MH I with limits obtained towards two other z 0:1 DLy systems, and show that SBS 1543+593 would not have been detected. Hence LSB galaxies similar to SBS 1543+593 can be responsible for DLy systems at even modest redshifts without being detectable from their 21-cm emission.en
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.title21-cm H I emission from the Damped Lyman-alpha absorber SBS 1543 593en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361:20010592
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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