Evolutionary self-consistent models of HII galaxies

Simple item page
dc.creatorManjón, M. Martín
dc.creatorMollá, M.
dc.creatorDíaz, A. I.
dc.date2007-01-26
dc.date.accessioned2026-07-07T08:46:58Z
dc.date.available2026-07-07T08:46:58Z
dc.descriptionWe have studied the viability of new theoretical models which combine a chemical evolution code, an evolutionary synthesis code and a photoionization code, to understand the star formation and evolution of H{\sc ii} galaxies. The emission lines observed in H{\sc ii} galaxies are reproduced by meas of the photoionization code CLOUDY, using as ionizing spectrum the spectral energy distribution of the modeled H{\sc ii} galaxy, which, in turn, is calculated according to a Star Formation History (SFH) and a metallicity evolution given by a chemical evolution model. Our technique reproduces the observed diagnostic diagrams and equivalent width-color correlations for local H{\sc ii} galaxies.
dc.description6 pages, 4 figures, contribution to the VII spanish astronomical society scientific meeeting (Barcelona, Spain)
dc.identifierhttps://arxiv.org/abs/astro-ph/0701757
dc.identifierhttp://arxiv.org/abs/astro-ph/0701757
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143435
dc.subjectAstrophysics
dc.titleEvolutionary self-consistent models of HII galaxies
dc.typetext

Files

Collections

arXiv