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An improved method to derive H I absorption spectra through the disks of galaxies - Application to the Sculptor Group

dc.contributor.authorDickey, J.M.
dc.contributor.authorBrinks, E.
dc.contributor.authorPuche, D.
dc.date.accessioned2009-01-08T15:50:16Z
dc.date.available2009-01-08T15:50:16Z
dc.date.issued1992
dc.identifier.citationDickey , J M , Brinks , E & Puche , D 1992 , ' An improved method to derive H I absorption spectra through the disks of galaxies - Application to the Sculptor Group ' , The Astrophysical Journal , vol. 385 , no. 1 , pp. 501-511 .
dc.identifier.issn0004-637X
dc.identifier.otherdspace: 2299/2775
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407951
dc.identifier.urihttp://hdl.handle.net/2299/2775
dc.descriptionOriginal article can be found at: http://adsabs.harvard.edu/abs/ Copyright American Astronomical Society [Full text of this article is not available in the UHRA]
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.titleAn improved method to derive H I absorption spectra through the disks of galaxies - Application to the Sculptor Groupen
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 (CAR)
dc.contributor.institutionRegistry
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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