Nuclear star formation in the hot-spot galaxy HGC 2903

dc.contributor.author	Alonso-Herrero, A.
dc.contributor.author	Ryder, S.D.
dc.contributor.author	Knapen, J.
dc.date.accessioned	2007-11-19T11:35:41Z
dc.date.available	2007-11-19T11:35:41Z
dc.date.issued	2000-06
dc.identifier.citation	Alonso-Herrero , A , Ryder , S D & Knapen , J 2000 , ' Nuclear star formation in the hot-spot galaxy HGC 2903 ' , Canada-France-Hawaii Telescope Information Bulletin , vol. 42 , pp. 16-17 . https://doi.org/10.1046/j.1365-8711.2001.04173.x
dc.identifier.other	dspace: 2299/1077
dc.identifier.uri	http://hdl.handle.net/2299/1077
dc.description	Original article can be found at : http://www.cfht.hawaii.edu/Reference/Bulletin/
dc.description.abstract	Circumnuclear regions (CNR) of enhanced star formation (SF) in disk galaxies are usually associated with the presence of stellar bars. Since bars are believed to be one of the most effective mechanisms for transporting material into the central regions of galaxies, CNRs are excellent laboratories for the study of the effects of inflow processes on the triggering of SF (see Knapen 1999 for a review on the subject).	en
dc.format.extent	30804
dc.language.iso	eng
dc.relation.ispartof	Canada-France-Hawaii Telescope Information Bulletin
dc.title	Nuclear star formation in the hot-spot galaxy HGC 2903	en
dc.contributor.institution	School of Physics, Astronomy and Mathematics
dc.description.status	Peer reviewed
rioxxterms.versionofrecord	10.1046/j.1365-8711.2001.04173.x
rioxxterms.type	Journal Article/Review
herts.preservation.rarelyaccessed	true