The warm interstellar gas in Starbursts and AGNs

Details The warm interstellar gas in Starbursts and AGNs The warm interstellar gas in Starbursts and AGNs

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007rmxac..29...80g&link_type=abstract

First Light Science with the GTC (Eds. R. Guzmán, C. Packham, J. M. Rodríguez-Espinosa, & S. Torres-Peimbert) Revista Mexicana d

Astronomy and Astrophysics

Astronomy

Galaxies: Active, Galaxies: Evolution, Galaxies: Starbursts, Ism

Scientific paper

Elucidating the relationship between intense star-formation and the AGN phenomenon is crucial to our understanding of the formation and evolution of galaxies and their SMBHs in the early universe. The warm interstellar gas is an excellent probe of the feedback processes taking place in galaxies, in particular in AGNs and starbursts. Deep imaging taken with OSIRIS tuned at the emission lines Lyα , CIV, HeII, Hα, and optical collisional lines of AGNs (Seyferts, Radio Galaxies and QSOs) and Starbursts (ULIRGs-VLIRGs) will help to determine whether there is an evolutionary link between star-formation and nuclear activity.

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