A Multi-Wave length Survey of the ISM in NGC 628

dc.contributor.author	Adler, D.S.
dc.contributor.author	Knapen, J.
dc.contributor.author	Fanelli, M.N.
dc.contributor.author	Westpfahl, D.
dc.contributor.author	Wakker, B.P.
dc.date.accessioned	2008-01-30T10:39:33Z
dc.date.available	2008-01-30T10:39:33Z
dc.date.issued	1999
dc.identifier.citation	Adler , 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.isbn	1-58381-007-2
dc.identifier.other	dspace: 2299/1465
dc.identifier.uri	http://hdl.handle.net/2299/1465
dc.description	Original paper can be found at http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific
dc.description.abstract	Is 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.format.extent	176307
dc.language.iso	eng
dc.publisher	Astronomical Society of the Pacific
dc.relation.ispartof	In: Galaxy Dynamics, ASP Conference Series vol.182
dc.title	A Multi-Wave length Survey of the ISM in NGC 628	en
dc.contributor.institution	School of Physics, Astronomy and Mathematics
rioxxterms.type	Other
herts.preservation.rarelyaccessed	true