Starbursts in H II Galaxies

dc.contributor.author	Brinks, E.
dc.date.accessioned	2008-02-14T13:41:00Z
dc.date.available	2008-02-14T13:41:00Z
dc.date.issued	1997
dc.identifier.citation	Brinks , E 1997 , ' Starbursts in H II Galaxies ' , Revista Mexicana de Astronomia y Astrofisica Serie de Conferencias, Vol. 6, vol. 1 , pp. 14-19 .
dc.identifier.other	dspace: 2299/1637
dc.identifier.other	ORCID: /0000-0002-7758-9699/work/30407929
dc.identifier.uri	http://hdl.handle.net/2299/1637
dc.description.abstract	H II galaxies fall at the lower end on the scale of the energy output of their starbursts. Still, they are genuine Starburst Galaxies, producing large numbers of massive stars, and at a rate which is unsustainable in the long term. In this contribution I discuss the effects of star formation on the interstellar medium in these dwarf galaxies, and review the possibility that interactions are responsible for the onset of the burst.	en
dc.format.extent	999634
dc.language.iso	eng
dc.relation.ispartof	Revista Mexicana de Astronomia y Astrofisica Serie de Conferencias, Vol. 6,
dc.title	Starbursts in H II Galaxies	en
dc.contributor.institution	School of Physics, Astronomy and Mathematics
dc.contributor.institution	School of Physics, Engineering & Computer Science
dc.contributor.institution	Department of Physics, Astronomy and Mathematics
dc.contributor.institution	Centre for Astrophysics Research (CAR)
dc.contributor.institution	Registry
dc.description.status	Peer reviewed
rioxxterms.type	Journal Article/Review
herts.preservation.rarelyaccessed	true