Through thick and thin: Kinematic and chemical components in the solar neighbourhood
We search for chemically distinct stellar components in the solar neighbourhood using a compilation of published data. Extending earlier work, we show that when the abundances of Fe, α elements and the r-process element Eu are considered together, stars
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Navarro_Through_thick_and_thin:_2011.pdf||798.31 kB||Adobe PDF|
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