English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We present chemical abundances of 15 stars in the {\gamma} Leo moving groupbased on high-resolution spectra with the Subaru High Dispersion Spectrograph.The sample was picked up by applying wavelet transform to UVW velocity compo-nents of stars in the solar neighbourhood. Both photometric and spectroscopicmethod have been used to determine the stellar parameters of stars. Abun-dances of 11 elements including Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni, Y and Baare measured. Our results show that the member stars display a wide metallicitydistribution with abundance ratios similar to Milky way disk stars. We presumethat the {\gamma} Leo moving group is originated from dynamical effectsprobably related to the Galactic spiral arms.

Tracing the origin of moving groups I. The {\gamma} Leo moving group with high resolution spectra from the Subaru Telescope