A new mid-infrared diagnostic between agn and starbursts
We present a new set of diagnostics which allow us to trace and classify in a statistical manner the mid-IR emission produced by active galactic nuclei (AGN) and star-forming regions. We construct a diagram based on the strength of the unidentified infrared band (UIB) at 6.2 μm, and the intensity of...
Guardado en:
Publicado: |
2001
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004640X_v276_n2-4_p569_Laurent http://hdl.handle.net/20.500.12110/paper_0004640X_v276_n2-4_p569_Laurent |
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