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Did globular clusters contribute to the stellar population of the Galactic halo?
C. Charbonnel,
M. Krause
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Research output
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Keyphrases
Globular Clusters
100%
Stellar Populations
100%
Galactic Halo
100%
Massive Stars
75%
Star Clusters
75%
Low-mass Stars
50%
Stellar Masses
25%
Clustering Features
25%
Milky Way
25%
Local Group
25%
Gas Mass
25%
Halo Stars
25%
Chemical Properties
25%
Initial Mass
25%
Local Group Galaxies
25%
Gas Expulsion
25%
Multiple Stellar Populations
25%
Early Infancy
25%
Dwarf Galaxies
25%
Physics
Galactic Halos
100%
Stellar Populations
100%
Globular Cluster
100%
Massive Star
75%
Star Cloud
75%
Low-Mass Star
50%
Dwarf Galaxy
25%
Local Galaxy Group
25%
Milky Way
25%
Halo Stars
25%
Stellar Mass
25%