Subarcsecond structure and velocity field of optical line-emitting gas in NGC 1052

Astrophysical Journal

Volumn 629, Issue 1 I, 2005, Pages 131-138

  Sugai, H ^a   Hattori, T ^b   Kawai, A ^a   Ozaki, S ^c   Kosugi, G ^b   Ohtani, H ^a,d   Hayashi, T ^e   Ishigaki, T ^f   Ishii, M ^g   Sasaki, M ^h   Takeyama, N ⁱ   Yutani, M ^b   Usuda, T ^b,j   Hayashi, S S ^b,j   Namikawa, K ^b  

^a KYOTO UNIVERSITY   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c Nishi Harima Astronomical Observatory   (Japan)

^d Toyama Science Museum ^*  (Japan)

^e Toyama Science Museum   (Japan)

^f HOKKAIDO UNIVERSITY   (Japan)

^g Kurashiki Science Center   (Japan)

^h SHIMONOSEKI CITY UNIVERSITY   (Japan)

ⁱ Mitaka Sangyo Plaza 601   (Japan)

^j GRADUATE UNIVERSITY FOR ADVANCED STUDIES   (Japan)

more..

Author keywords

Galaxies: active; Galaxies: individual (NGC 1052); Galaxies: ISM; Galaxies: kinematics and dynamics; Galaxies: nuclei

Indexed keywords

EID: 28144462013     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/431544     Document Type: Article

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