Formation of bulges in very late-type galaxies from super star clusters

Monthly Notices of the Royal Astronomical Society

Volumn 339, Issue 2, 2003, Pages 442-446

  Fu, Y N ^a,b,c   Huang, J H ^d   Deng, Z G ^e  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b Institut de Mecanique Celeste et de Calcul des ephemerides   (France)

^c INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

^d NANJING UNIVERSITY   (China)

^e UNIVERSITY OF CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Galaxies: bulges; Galaxies: kinematics and dynamics; Galaxies: star clusters

Indexed keywords

ASTROPHYSICS; STARS;

CLUSTER MOVING; DARK MATTER HALOS; DENSITY PROFILE; DYNAMICAL EVOLUTION; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES: STAR CLUSTERS; GALAXY:BULGE; LATE-TYPE; PHYSICAL PROCESS; STAR CLUSTERS;

GALAXIES;

EID: 0142073789     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06177.x     Document Type: Article

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