Spectral Lines in the Ca ii Triplet Region for RAVE DR6 Chemical Abundance Pipeline
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چکیده
منابع مشابه
Using the Ca II Triplet to Trace Abundance Variations in Individual Red Giant Branch stars in Three Nearby Galaxies
Spectroscopic abundance determinations for stars spanning a Hubble time in age are necessary in order to unambiguously determine the evolutionary histories of galaxies. Using FORS1 in Multi-Object Spectroscopy mode on ANTU (UT1) at the ESO-VLT on Paranal we obtained near infrared spectra from which we measured the equivalent widths of the two strongest Ca II triplet lines to determine metal abu...
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ژورنال
عنوان ژورنال: Research Notes of the AAS
سال: 2018
ISSN: 2515-5172
DOI: 10.3847/2515-5172/aaf0fa