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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2165
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dc.contributor.authorRavindranath, S-
dc.contributor.authorPrabhu, T. P-
dc.date.accessioned2008-03-28T09:10:04Z-
dc.date.available2008-03-28T09:10:04Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 407 - 408en
dc.identifier.urihttp://hdl.handle.net/2248/2165-
dc.description.abstractBased on the optical-NIR spectra, we discuss the nebular properties and stellar populations of starburst nuclei. Starbursts are found to have higher electron densities and higher excitations compared to HII nuclei. We find evidence for a composite population of young, ionizing massive stars (less than 3 Myr old) co-existing with the evolved RSG populations (about 5 to 7 Myr old) in most of our sample starburst nuclei.en
dc.format.extent184474 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..407Ren
dc.subjectStarburst galaxiesen
dc.subjectHII nucleien
dc.subjectEmission linesen
dc.titleStudy of the emission line spectra and the stellar populations of starburst galaxiesen
dc.typeArticleen
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