Molecular gas in NUclei of GAlaxies (NUGA). I. The counter-rotating LINER NGC 4826

Astronomy and Astrophysics

Volumn 407, Issue 2, 2003, Pages 485-502

  Garcia Burillo S ^a   Combes, F ^b   Hunt, L K ^c   Boone, F ^d   Baker, A J ^e   Tacconi, L J ^e   Eckart, A ^f   Neri, R ^g   Leon, S ^h   Schinnerer, E ⁱ   Englmaier, P ^j  

^a Observatorio de Madrid   (Spain)

^b OBSERVATOIRE DE PARIS   (France)

^c INAF ISTITUTO DI RADIOASTRONOMIA   (Italy)

^d RUHR UNIVERSITY BOCHUM   (Germany)

^e MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^f UNIVERSITY OF COLOGNE   (Germany)

^g IRAM   (France)

^h INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

ⁱ NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^j UNIVERSITY OF BASEL   (Switzerland)

more..

Author keywords

Galaxies: individual: NGC 4826; Galaxies: ISM; Galaxies: kinematics and dynamics; Galaxies: nuclei; Radio lines: galaxies

Indexed keywords

GALAXIES; GASES; INTERFEROMETERS; KINEMATICS; PERTURBATION TECHNIQUES;

ACTIVE GALACTIC NUCLEI; GAS KINEMATICS; GRAVITATIONAL TORQUES; MOLECULAR GAS;

ASTRONOMY;

EID: 0043062617     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030866     Document Type: Article

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