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http://dx.doi.org/10.5303/PKAS.2012.27.4.295

NEAR-INFRARED HIGH-RESOLUTION SPECTROSCOPY OF THE OBSCURED AGN IRAS 01250+2832  

Shirahata, M. (Department of Space Astronomy and Astrophysics, ISAS/JAXA)
Usuda, T. (Subaru Telescope, NAOJ)
Oyabu, S. (Nagoya University)
Nakagawa, T. (Department of Space Astronomy and Astrophysics, ISAS/JAXA)
Yamamura, I. (Department of Space Astronomy and Astrophysics, ISAS/JAXA)
Publication Information
Publications of The Korean Astronomical Society / v.27, no.4, 2012 , pp. 295-296 More about this Journal
Abstract
We provide a new physical insight on the hot molecular clouds near the nucleus of the heavily obscured AGN IRAS 01250+2832, based on the results of near-infrared high-resolution spectroscopy of gaseous CO ro-vibrational absorption lines with Subaru/IRCS. The detected CO absorption lines up to highly excited rotational levels reveal that hot dense molecular clouds exist around the AGN under the peculiar physical conditions.
Keywords
galaxies: active; galaxies: nuclei; galaxies: individual (IRAS 01250+2832); galaxies: ISM; infrared: galaxies;
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  • Reference
1 Shirahata, M., et al., 2012, Infrared Spectroscopy of CO Ro-vibrational Absorption Lines toward the Obscured AGN IRAS 08572+3915, PASJ, accepted
2 Shirahata, M., 2006, Probing Molecular Tori in Obscured Active Galactic Nuclei with Spectroscopic Observations of CO Ro-vibrational Absorption Lines, Ph.D. thesis, University of Tokyo
3 Oyabu, S., et al., 2011, AKARI Detections of Hot Dust in Luminous Infrared Galaxies: Search for Dusty Active Galactic Nuclei, A&A, 529, A122   DOI   ScienceOn