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- 2022
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Mark
An old, metal-rich accreted stellar component in the Milky Way stellar disk
(
- Contribution to journal › Article
- 2020
-
Mark
The HR 1614 moving group is not a dissolving cluster
(
- Contribution to journal › Article
- 2019
-
Mark
The Gaia-ESO survey: Calibrating a relationship between age and the [C/N] abundance ratio with open clusters?
(
- Contribution to journal › Article