A multiwavelength vision of star forming regions: What does lambda_1 know about lambda_2?

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dc.creatorCervino, M.
dc.date2002-10-14
dc.date.accessioned2026-07-07T02:05:42Z
dc.date.available2026-07-07T02:05:42Z
dc.descriptionIn this contribution I show the physical limitations to the application of standard synthesis models from 0 to 10 Gyr. I also present the multiwavelength spectrum (from gamma-rays to radio) of young star forming regions based on evolutionary population synthesis models that takes into account the stochasticity of the star formation proces. I show how the correlation of different observables can allow to establish a better understanding of the star formation processes. Finally I compare the spectral energy distribution of AGNs and star forming regions and I show the possible connection of Star Forming Galaxies with Seyfert 2 AGNs.
dc.description6 pages, 3 figures, to appear in "Star Formation through Time", Perez, Gonzalez Delgado and Tenorio-Tagle (eds.) ASP Conference Series (2003)
dc.identifierhttps://arxiv.org/abs/astro-ph/0210312
dc.identifierhttp://arxiv.org/abs/astro-ph/0210312
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5181
dc.subjectAstrophysics
dc.titleA multiwavelength vision of star forming regions: What does lambda_1 know about lambda_2?
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