THE 3.3 MICRON PAH EMISSION OF THE MID-INFRARED EXCESS GALAXIES DISCOVERED BY THE AKARI MID-INFRARED ALL-SKY SURVEY |
Yamada, R.
(Graduate school of science, Nagoya University)
Oyabu, S. (Graduate school of science, Nagoya University) Kaneda, H. (Graduate school of science, Nagoya University) Yamagishi, M. (Graduate school of science, Nagoya University) Ishihara, D. (Graduate school of science, Nagoya University) Kim, J.H. (Department of Physics and Astronomy, Seoul National University) Im, M. (Department of Physics and Astronomy, Seoul National University) Toba, Y. (Institute of Space and Astronomical Science, Japan Aerospace Exploration Agency) Matsuhara, H. (Institute of Space and Astronomical Science, Japan Aerospace Exploration Agency) |
1 | Sanders, D. B. & Mirabel, I. F., 1996, Luminous Infrared Galaxies, ARA&A, 34, 749 DOI ScienceOn |
2 | Imanishi, M., et al., 2008, Systematic Infrared 2.5- 5 Spectroscopy of Nearby Ultraluminous Infrared Galaxies with AKARI, PASJ, 60, S489 |
3 | Imanishi, M., et al., 2010, AKARI IRC Infrared 2.5-5 Spectroscopy of a Large Sample of Luminous Infrared Galaxies, ApJ, 721, 1233 DOI |
4 | Moorwood, A. F. M., 1986, 3.28 Micron Feature and Continuum Emission in Galaxy Nuclei, A&A, 166, 4 |
5 | Mouri, H., et al., 1990, A Relation between H2 V = 1-0 S(1) and 3.28 Micron Emission in Seyfert and Starburst Galaxies, ApJ, 356, L39 DOI |
6 | Oyabu, S., et al. 2011, AKARI Detections of Hot Dust in Luminous Infrared Galaxies. Search for Dusty Active Galactic Nuclei, A&A 529, 122 DOI ScienceOn |