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PAH EMISSION IN STARBURST, SEYFERT, ULIRGS, QSOS AND QUASAR OBJECTS, AND THEIR RELATION WITH THE INFRARED, X-RAY AND RADIO CONTINUUM EMISSION

This is a second study in an ongoing work aimed to analyze the star formation activity and its relation with the Polycyclic Aromatic Hydrocarbon (PAHs) emission. In this way, we have performed a study about the correlation between the ux of the 7.7 -m PAH band and its equivalent width, with the lum...

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Publicat a:Revista Mexicana de Astronomía y Astrofísica
Autors principals: M.-A. Higuera-G., A. Rodríguez-Ardila, J. M. Tejeiro S.
Format: Artigo
Idioma:Inglês
Publicat: Universidad Nacional Autónoma de México 2009
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Accés en línia:https://www.redalyc.org/articulo.oa?id=57115758085
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