Why the Canis Major overdensity is not due to the Warp: Analysis of its radial profile and velocities

Monthly Notices of the Royal Astronomical Society

Volumn 355, Issue 4, 2004, Pages

  Martin, N F ^a   Ibata, R A ^a   Conn, B C ^b   Lewis, G F ^b   Bellazzini, M ^c   Irwin, M J ^d   McConnachie, A W ^d  

^a OBSERVATOIRE DE STRASBOURG   (France)

^b UNIVERSITY OF SYDNEY   (Australia)

^c OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^d UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

Galaxies: interactions; Galaxy: formation; Galaxy: structure

Indexed keywords

GALAXIES; VELOCITY;

GALACTIC DISKS; GALAXIES: INTERACTIONS; GALAXIES:STRUCTURE; GALAXY FORMATIONS; LOW DISPERSIONS; NORTHERN HEMISPHERES; RADIAL DISTRIBUTIONS; RADIAL PROFILES; RADIAL VELOCITY; STELLAR POPULATIONS;

GIANT STARS;

EID: 11144311972     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08521.x     Document Type: Article

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