Crossref Citations
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Freeman, K. C.
2013.
Local Group Cosmology.
p.
1.
Published online by Cambridge University Press: 07 August 2017
Kinematics and abundances have been determined for a large sample of K giants in a field at ∼2 kpc from the center to study the relationship between the bulge and the halo. There are two different kinematic groups evident. The metal-poor stars have low rotation and high velocity dispersion, and so can be associated with the halo. The metal-richer stars have intermediate rotation. Our data suggest that the bulge and halo could be separate kinematical entities.