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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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| Yayımlandı: | Revista Mexicana de Astronomía y Astrofísica |
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| Asıl Yazarlar: | , , |
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
Universidad Nacional Autónoma de México
2009
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| Konular: | |
| Online Erişim: | https://www.redalyc.org/articulo.oa?id=57115758085 |
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