Why does NGC 1068 have a more powerful active galactic nucleus than NGC 4258?

Publications of the Astronomical Society of Japan

Volumn 49, Issue 4, 1997, Pages

  Murayama, Takashi ^a   Taniguchi, Yoshiaki ^a  

^a TOHOKU UNIVERSITY   (Japan)

Author keywords

Galaxies: individual (NGC 1068, NGC 4258); Galaxies: internal motions; Galaxies: nuclei; Galaxies: seyfert; Masers

Indexed keywords

ENGINES; MASERS; STARS;

ACTIVE GALACTIC NUCLEI; CENTRAL ENGINES; GALAXIES:INDIVIDUAL:NGC 1068; GALAXIES:NUCLEI; GALAXY: INDIVIDUAL (NGC 1068, NGC 4258); GALAXY: INTERNAL MOTION; GALAXY:SEYFERT; INTERNAL MOTION; MASER EMISSIONS; WATER VAPOUR;

GALAXIES;

EID: 0031286757     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/49.4.L13     Document Type: Article

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