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dc.contributor.authorAdler, D.S.
dc.contributor.authorKnapen, J.
dc.contributor.authorFanelli, M.N.
dc.contributor.authorWestpfahl, D.
dc.contributor.authorWakker, B.P.
dc.date.accessioned2008-01-30T10:39:33Z
dc.date.available2008-01-30T10:39:33Z
dc.date.issued1999
dc.identifier.citationAdler , D S , Knapen , J , Fanelli , M N , Westpfahl , D & Wakker , B P 1999 , A Multi-Wave length Survey of the ISM in NGC 628 . in In: Galaxy Dynamics, ASP Conference Series vol.182 . Astronomical Society of the Pacific , pp. 227-228 .
dc.identifier.isbn1-58381-007-2
dc.identifier.otherPURE: 171278
dc.identifier.otherPURE UUID: 6aea99b2-c485-4cde-869b-edb663ac6d25
dc.identifier.otherdspace: 2299/1465
dc.identifier.urihttp://hdl.handle.net/2299/1465
dc.descriptionOriginal paper can be found at http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific
dc.description.abstractIs atomic hydrogen a precursor to or byproduct of the star formation process? Recent evidence suggests that a large percentage of the atomic hydrogen in spiral galaxies could be due to photodissociation of molecular gas by UV radiation from hot young stars.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Galaxy Dynamics, ASP Conference Series vol.182
dc.rightsOpen
dc.titleA Multi-Wave length Survey of the ISM in NGC 628en
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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