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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S315(11), 2015

DOI: 10.1017/s1743921316008334

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Molecular Gas Excitation and Chemistry in VV 114 and NGC 1614 with ALMA

Journal article published in 2015 by Toshiki Saito, Daisuke Iono, Junko Ueda, Min S. Yun, Kouichiro Nakanishi, Hajime Sugai, Masatoshi Imanishi, Yoshiaki Hagiwara, Hiroyuki Kaneko ORCID, Kentaro Motohara, Daniel Espada ORCID, Takuji Yamashita, Minju Lee, Tomonari Michiyama, Ryohei Kawabe
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe present high resolution molecular line observations of dusty AGN and starburst in nearby luminous infrared galaxies (LIRGs), VV 114 (band 3/4/7) and NGC 1614 (band 3/6/7/9), with ALMA. Multi-frequency imaging from 4.8 GHz to 691 GHz of NGC 1614 allows us to study spatial properties of the radio-to-FIR continuum and multiple CO transitions, and we find the CO excitation up to Jupp = 6 can be explained by a single ISM model powered by nuclear starbursts. Our processing line imaging survey for VV 114 detected at least 30 molecular lines which show different chemical composition from region to region. Multi-molecule imaging helps us to diagnose the chemical differences of dusty ISM, while multi-transition imaging allows us to investigate gas physical conditions affected by nuclear activities directly.

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