Axisymmetric dynamical models for SAURON and OASIS observations of NGC 3377

Astronomy and Astrophysics

Volumn 415, Issue 3, 2004, Pages 889-903

  Copin, Y ^a,d   Cretton, N ^b,e   Emsellem, E ^c  

^a Lyon Medicine University   (France)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

^d LEIDEN UNIVERSITY   (Netherlands)

^e MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Galaxies: individual: NGC 3377; Galaxies: kinematics and dynamics

Indexed keywords

ASTROPHYSICS; COMPUTER SIMULATION; KINEMATICS; OPTICAL RESOLVING POWER; SPACE OPTICS; SPECTROGRAPHS; SPECTROSCOPY;

AXISYMMETRIC DYNAMICAL MODEL; SCHWARZSCHILD NUMERICAL ORBIT SUPERPOSITION TECHNIQUE;

GALAXIES;

EID: 1542366471     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034076     Document Type: Article

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