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dc.contributor.authorWalter, F.
dc.contributor.authorBrinks, E.
dc.date.accessioned2008-01-30T10:45:19Z
dc.date.available2008-01-30T10:45:19Z
dc.date.issued1999
dc.identifier.citationWalter , F & Brinks , E 1999 , VLA HI imaging of the Low Surface Brightness dwarf galaxy DDO47 . in In: Procs of Low Surface Brightness Universe, ASP Conference Series 170 . Astronomical Society of the Pacific , pp. 224-228 .
dc.identifier.isbn1-886733-92-9
dc.identifier.otherPURE: 142401
dc.identifier.otherPURE UUID: 68b8bdfe-e588-4aa5-a1d2-8ed7b278b103
dc.identifier.otherdspace: 2299/1498
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407910
dc.identifier.urihttp://hdl.handle.net/2299/1498
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 VLA-observations of the nearby Low Surface Brightness Galaxy DDO 47. This object shows many hole-like structures in its neutral interstellar medium. The majority of the detected H I-shells are found to be expanding. Their origin is therefore believed to be due to stellar winds of the most massive stars and their subsequent supernova (SN type II) explosions within regions of recent star formation.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Low Surface Brightness Universe, ASP Conference Series 170
dc.rightsOpen
dc.titleVLA HI imaging of the Low Surface Brightness dwarf galaxy DDO47en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1999
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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