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dc.contributor.authorBrinks, E.
dc.date.accessioned2008-02-14T13:41:00Z
dc.date.available2008-02-14T13:41:00Z
dc.date.issued1997
dc.identifier.citationBrinks , 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.otherPURE: 150040
dc.identifier.otherPURE UUID: baf6d147-2038-427c-9648-c1d3a4883cbd
dc.identifier.otherdspace: 2299/1637
dc.identifier.otherScopus: 25844466143
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407929
dc.identifier.urihttp://hdl.handle.net/2299/1637
dc.description.abstractH 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.language.isoeng
dc.relation.ispartofRevista Mexicana de Astronomia y Astrofisica Serie de Conferencias, Vol. 6,
dc.titleStarbursts in H II Galaxiesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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