dc.contributor.author | Knapen, J. | |
dc.contributor.author | Beckman, J.E. | |
dc.date.accessioned | 2008-02-05T12:10:40Z | |
dc.date.available | 2008-02-05T12:10:40Z | |
dc.date.issued | 1994 | |
dc.identifier.citation | Knapen , J & Beckman , J E 1994 , The Role of HI in the Star-Formation Processes in Spiral Disks . in In: Physics of the Gaseous and Stellar Disks of the Galaxy - ASP Conf Series 66 . Astronomical Society of the Pacific , pp. 329-336 . | |
dc.identifier.isbn | 0-937707-85-6 | |
dc.identifier.other | PURE: 146833 | |
dc.identifier.other | PURE UUID: 9f542cfe-432d-40ef-bbc9-16371608b0bc | |
dc.identifier.other | dspace: 2299/1553 | |
dc.identifier.uri | http://hdl.handle.net/2299/1553 | |
dc.description | Original paper can be found at: http://www.astrosociety.org/pubs/cs/035-069.html | |
dc.description.abstract | We discuss recent work on massive star-formation efficiency parameters on 1 kpc scales in grand-design spiral galaxies. The fact that in two galaxies studies in detail, M51 and NGC 4321, the massive star-formation efficiency in the arms is larger than that outside the arms can be seen as evidence for large-scale triggering of the star formation in the arms, probably induced by a density wave system. We discuss several possible systematic effects, but infer that the conclusions on triggering are sound. | en |
dc.language.iso | eng | |
dc.publisher | Astronomical Society of the Pacific | |
dc.relation.ispartof | In: Physics of the Gaseous and Stellar Disks of the Galaxy - ASP Conf Series 66 | |
dc.title | The Role of HI in the Star-Formation Processes in Spiral Disks | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |