CN anomalies in the halo system and the origin of globular clusters in the Milky Way
We explore the kinematics and orbital properties of a sample of red giants in the halo system of the Milky Way that are thought to have formed in globular clusters based on their anomalously strong UV/blue CN bands. The orbital parameters of the CN-strong
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Carollo_CN_anomalies_in_the_halo_2013.pdf||2.57 MB||Adobe PDF|
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