Spectrophotometric Evolutionary Models for Tidal Dwarfs

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dc.creatorWeilbacher, Peter M.
dc.creatorAlvensleben, Uta Fritze-v.
dc.date2001-05-16
dc.date.accessioned2026-07-07T01:58:35Z
dc.date.available2026-07-07T01:58:35Z
dc.descriptionWe describe our procedure to model Tidal Dwarf Galaxies in the context of our evolutionary synthesis code. Our analysis shows strong contributions of gaseous emission lines to optical colors and of continuum emission to NIR colors during the burst phase. This underlines the importance of including both types of emission when modeling any type of star-bursting galaxies.
dc.descriptionTo be published in: ``Dwarf Galaxies and their Environment'', eds. K.S. de Boer, R.-J. Dettmar, U. Klein
dc.identifierhttps://arxiv.org/abs/astro-ph/0105272
dc.identifierhttp://arxiv.org/abs/astro-ph/0105272
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2773
dc.subjectAstrophysics
dc.titleSpectrophotometric Evolutionary Models for Tidal Dwarfs
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