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We explore the kinematics and orbital properties of a sample of red giants inthe halo system of the Milky Way that are thought to have formed in globularclusters, based on their anomalously strong UV/blue CN bands. The orbitalparameters of the CN-strong halo stars are compared to those of the inner- andouter-halo populations as described by Carollo et al., and to the orbitalparameters of globular clusters with well-studied Galactic orbits. TheCN-strong field stars and the globular clusters both exhibit kinematics andorbital properties similar to the inner-halo population, indicating thatstripped or destroyed globular clusters could be a significant source ofinner-halo field stars, and suggesting that both the CN-strong stars and themajority of globular clusters are primarily associated with this population.

CN Anomalies in the Halo System and the Origin of Globular Clusters in the Milky Way