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The nature of the Milky Way's stellar halo revealed by the three integrals of motion
Free accessArXiv | 2020| -
CARBON-ENHANCED METAL-POOR STARS: CEMP-s and CEMP-no SUBCLASSES IN THE HALO SYSTEM OF THE MILKY WAY
Online Contents | 2014| -
CN ANOMALIES IN THE HALO SYSTEM AND THE ORIGIN OF GLOBULAR CLUSTERS IN THE MILKY WAY
Online Contents | 2013| -
CARBON-ENHANCED METAL-POOR STARS IN THE INNER AND OUTER HALO COMPONENTS OF THE MILKY WAY
Online Contents | 2012| -
CARBON-ENHANCED METAL-POOR STARS IN THE INNER AND OUTER HALO COMPONENTS OF THE MILKY WAY
Online Contents | 2012| -
CARBON-ENHANCED METAL-POOR STARS IN THE INNER AND OUTER HALO COMPONENTS OF THE MILKY WAY
Online Contents | 2012| -
The Assembly of the Halo System of the Milky Way as Revealed by SDSS/SEGUE -- The CEMP Star Connection
Free accessArXiv | 2011| -
Searches for the Most Metal‐Poor Candidates from SDSS and SEGUE
American Institute of Physics | 2008| -
Understanding the early stages of galaxy formation using very metal-poor stars from the Hamburg/ESO survey
Free accessArXiv | 2022| -
CN Anomalies in the Halo System and the Origin of Globular Clusters in the Milky Way
Free accessArXiv | 2013| -
Extreme Enhancements of r-process Elements in the Cool Metal-Poor Main-Sequence Star SDSS J2357-0052
Free accessArXiv | 2010|
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