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The Connection between Starburst and AGN Activities Probed with the 3.3μm PAH Emission

Published online by Cambridge University Press:  21 March 2013

Ji Hoon Kim ,
M. Im ,
J.-H. Woo  and
D. Kim
Ji Hoon Kim
Affiliation:
National Research Foundation of Korea Postdoctoral Fellow Center for the Exploration of the Origin of the Universe, SNU, Korea Department of Physics and Astrnomy, Seoul National University, Seoul 151-747, Korea email: jhkim@astro.snu.ac.kr
M. Im
Affiliation:
Center for the Exploration of the Origin of the Universe, SNU, Korea Department of Physics and Astrnomy, Seoul National University, Seoul 151-747, Korea email: jhkim@astro.snu.ac.kr
J.-H. Woo
Affiliation:
Department of Physics and Astrnomy, Seoul National University, Seoul 151-747, Korea email: jhkim@astro.snu.ac.kr
D. Kim
Affiliation:
Center for the Exploration of the Origin of the Universe, SNU, Korea Department of Physics and Astrnomy, Seoul National University, Seoul 151-747, Korea email: jhkim@astro.snu.ac.kr
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Abstract

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We investigated the connection between AGN and star formation (SF) activities of various kinds of AGNs and their host galaxies. In order to probe SF activity, we measured the 3.3 μm PAH emission luminosity utilizing the slitless spectroscopic capability of AKARI space telescope. We present the results from two missions, ASCSG and LQSONG.

Keywords

galaxies: active — galaxies: starburst — galaxies: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 191
Copyright
Copyright © International Astronomical Union 2013