Ionising stellar populations in circumnuclear star forming regions

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dc.creatorPerez-Montero, Enrique
dc.creatorDiaz, Angeles I.
dc.creatorCastellanos, Marcelo
dc.date2004-11-10
dc.date.accessioned2026-07-07T02:15:45Z
dc.date.available2026-07-07T02:15:45Z
dc.descriptionWe present a study of the stellar populations and gas physical conditions in Circumnuclear Star Forming Regions (CNSFRs) based on spectrophotometric data, including the 7000 angstroms to 1 micron spectral range, which is of great interest to the whole diagnostic of the ionized gas. The properties of CNSFRs as a class are inferred from a comparison with those of other star forming emission-line objects: low excitation disc HII regions and HII galaxies.
dc.description6 pages, 4 eps figures. Proceeding for the conference "Starbursts: From 30 Doradus to Lyman Break Galaxies", held in Cambridge (UK) in September, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0411278
dc.identifierhttp://arxiv.org/abs/astro-ph/0411278
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8529
dc.subjectAstrophysics
dc.titleIonising stellar populations in circumnuclear star forming regions
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