Nobeyama millimeter array observations of luminous infrared galaxies
EAS Publications Series, ISSN: 1633-4760, Vol: 31, Page: 93-96
2008
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Conference Paper Description
We present the results of systematic millimeter interferometric observations of luminous infrared galaxies (LIRGs), using the Nobeyama Millimeter Array. We observed HCN (J = 1-0) and HCO (J = 1-0) emission lines simultaneously, and derived their brightness-temperature ratios, to investigate whether the observed ratios are similar to those found in AGN-dominated nuclei or starburst galaxies. LIRGs with (without) luminous buried AGN signatures in our infrared spectra tend to show high (low) HCN (J = 1-0) to HCO (J = 1-0) brightness-temperature ratios as seen in galaxy nuclei dominated by AGNs (starbursts). The high ratios in buried AGN candidates could be explained by the enhanced HCN abundance, and/or infrared radiative pumping of the HCN molecule, in the close vicinity of an AGN. © 2008 EAS EDP Sciences.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=53349090555&origin=inward; http://dx.doi.org/10.1051/eas:0831019; http://www.eas-journal.org/10.1051/eas:0831019; http://www.eas-journal.org/10.1051/eas:0831019/pdf; http://dx.doi.org/10.1051/eas%3A0831019; https://dx.doi.org/10.1051/eas%3A0831019; https://www.eas-journal.org/articles/eas/abs/2008/04/eas0831018/eas0831018.html
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