Massive Star Forming Regions: from diagnostic tools to derived properties

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dc.creatorSchaerer, Daniel
dc.date2000-07-20
dc.date.accessioned2026-07-07T01:54:28Z
dc.date.available2026-07-07T01:54:28Z
dc.descriptionThe current state-of-the-art of multi-wavelength diagnostic tools (evolutionary synthesis, photoionisation models) for massive star forming regions (HII regions, starbursts, etc.) and some of their input physics (especially model atmospheres) is reviewed. Analysis of stellar populations based on integrated spectra from both stellar features and nebular emission lines from the UV to IR are summarised. We stress the importance of "template" studies at various scales (from individual stars to well studied galaxies) and various wavelengths, to understand the processes operating in massive star forming regions and to reliably derive their properties.
dc.descriptionto appear in "Stars, Gas and Dust in Galaxies: Exploring the Links", Eds. D. Alloin, G. Galaz, K. Olsen, ASP Conf. Series, in press. 9 pages, including 1 figure. Related preprints also available at http://webast.ast.obs-mip.fr/people/schaerer/Preprints.html
dc.identifierhttps://arxiv.org/abs/astro-ph/0007307
dc.identifierhttp://arxiv.org/abs/astro-ph/0007307
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1364
dc.subjectAstrophysics
dc.titleMassive Star Forming Regions: from diagnostic tools to derived properties
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