Elemental abundances in Hyades supercluster (De Silva+, 2011)

Details Elemental abundances in Hyades supercluster (De Silva+, 2011) Elemental abundances in Hyades supercluster (De Silva+, 2011)

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ycat..74150563d&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/415/563. Originally published in: 2011MNRAS.415..563D

Computer Science

Clusters: Open, Stars: Nearby, Abundances

Scientific paper

High-resolution and high signal-to-noise ratio spectra of probable members of the Hyades supercluster were observed using the VLT UV-Visual Echelle Spectrograph (UVES) at UT2 in the framework of programmes 080.D-0094(A) and 381.B-0045(A). A total of 45 probable member stars were submitted for service mode observations, using the UVES Red arm standard setting at 520 nm which provides complete spectral coverage from 4200 to 6200Å, and employed a 0.8-arcsec slit to achieve a spectral resolving power of 60000.
(3 data files).

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