Luminous HC3N line and the HCN/HCO+ ratio in NGC 4418 Buried AGN or nascent starburst?

Astronomy and Astrophysics

Volumn 475, Issue 2, 2007, Pages 479-485

  Aalto, S ^a   Monje, R ^a   Martin S ^b  

^a CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Galaxies: active; Galaxies: evolution; Galaxies: individual: NGC 4418; Galaxies: starburst; ISM: molecules; Radio lines: ISM

Indexed keywords

GALAXIES; HYDROGEN INORGANIC COMPOUNDS; INFRARED RADIATION; LUMINANCE; POSITIVE IONS; RADIATIVE TRANSFER;

GALAXIES: EVOLUTION; GALAXIES: STARBURST; MOLECULAR CHEMISTRY; RADIO LINES: ISM;

STARS;

EID: 36549024956     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20077366     Document Type: Article

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