Tracing the Origin of Moving Groups. I. The γ Leo Moving Group with High-resolution Spectra from the Subaru Telescope

We present chemical abundances of 15 stars in the γ Leo moving group based on high-resolution spectra with the Subaru High Dispersion Spectrograph. The sample was picked up by applying wavelet transform to UVW velocity components of stars in the solar neighborhood. Both photometric and spectroscopic...

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Veröffentlicht in:	The Astrophysical journal 2018-08, Vol.863 (1), p.4
Hauptverfasser:	Liang, X. L., Zhao, J. K., Zhao, G., Aoki, W., Ishigaki, M. N., Matsuno, T., Chen, Y. Q., Kong, X. M., Shi, J. R., Xing, Q. F.
Format:	Artikel
Sprache:	eng
Schlagworte:	Abundance Aluminum Astrophysics Chromium Galactic structure High resolution Magnesium Metallicity Milky Way Nickel Organic chemistry Reflecting telescopes Silicon Solar neighborhood Stars stars: abundances stars: kinematics and dynamics Titanium Wavelet transforms
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