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Detailed chemical abundances for twenty one elements are presented for four red giants in the anomalous outer halo globular cluster Palomar 1 ($R_{\rm{GC}} = 17.2$ kpc, $Z=3.6$ kpc) using high-resolut...
\epsilon Auriga is one of the most mysterious objects on the sky. Prior modeling of its light-curve assumed a dark, inclined, non-transparent or semi-transparent, dusty disk with a central hole. The h...
Motivated by observations that only a very few stars have been found to have antisolar differential rotation, much weaker in amplitude than that of the Sun, we analyze the stability of antisolar and s...
The delayed contribution of low and intermediate mass stars to chemical galactic enrichment:an analytical approach。
A Chemical Abundance Study of three RHB and two RGB stars in NGC 6637 (M69)。
Elemental abundance studies of CP stars. The silicon stars HD 87240 and HD 96729。

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