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dc.contributor.authorTaylor, C.L.
dc.contributor.authorBrinks, E.
dc.contributor.authorSkillman, E.D.
dc.date.accessioned2008-01-30T10:45:18Z
dc.date.available2008-01-30T10:45:18Z
dc.date.issued1999
dc.identifier.citationTaylor , C L , Brinks , E & Skillman , E D 1999 , HI properties of Low Surface Brightness dwarf and blue compact dwarf galaxies . in In: Procs of Low Surface Brightness Universe, IAU Colloquium 171, ASP Conference Series 170 . Astronomical Society of the Pacific , pp. 337-339 .
dc.identifier.isbn1-886733-92-9
dc.identifier.otherPURE: 142937
dc.identifier.otherPURE UUID: 616f50cd-44c8-4cb7-a4ad-a6e5da6a1b05
dc.identifier.otherdspace: 2299/1497
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407919
dc.identifier.urihttp://hdl.handle.net/2299/1497
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe present high resolution (~15") VLA HI observations of one LSB dwarf galaxy and 5 Blue Compact Dwarfs. Previous works have emphasized the difference in the peak column density of the HI between the two types of galaxy. However, the peak column density is typically only a factor of 2-4 greater in BCDs than in LSB dwarfs, suggesting that the difference between the two is one of degree, not quality. The HI morphologies of the two types are often quite similar.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Low Surface Brightness Universe, IAU Colloquium 171, ASP Conference Series 170
dc.titleHI properties of Low Surface Brightness dwarf and blue compact dwarf galaxiesen
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
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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