High-resolution elemental abundance analysis of the Hyades supercluster
The existence of a kinematically defined moving group of stars centred at U=-40,V=-17 kms-1, referred to as the Hyades supercluster, has been suggested to be the debris of an originally large star-forming event, with its core being the present-day Hyades
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|Access Rights:||Open Access|
|01_De Silva_High-resolution_elemental_2011.pdf||719.63 kB||Adobe PDF|
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