Probing circumnuclear environments with the HCN(J= 3-2) and HCO +(J= 3-2) lines: Case of NGC 1097

Astrophysical Journal

Volumn 747, Issue 2, 2012, Pages

  Hsieh, Pei Ying ^a,b   Ho, Paul T P ^a,c   Kohno, Kotaro ^d,e   Hwang, Chorng Yuan ^b   Matsushita, Satoki ^a,f  

^a INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^b NATIONAL CENTRAL UNIVERSITY   (Taiwan)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIVERSITY OF TOKYO   (Japan)

^e UNIVERSITY OF TOKYO   (Japan)

^f JOINT ALMA OBSERVATORY   (Chile)

Author keywords

galaxies: individual (NGC 1097); galaxies: ISM; galaxies: Seyfert; ISM: molecules; radio lines:ISM; submillimeter: ISM

Indexed keywords

EID: 84859707222     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/747/2/90     Document Type: Article

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