Averaged [Fe/H] for Cool Dwarfs (Taylor, 1995)

Details Averaged [Fe/H] for Cool Dwarfs (Taylor, 1995) Averaged [Fe/H] for Cool Dwarfs (Taylor, 1995)

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ycat.5088....0t&link_type=abstract

VizieR On-line Data Catalog: V/88. Originally published in: 1994PASP..106..704T; 1995PASP..107..734T

Physics

3

Abundances: [Fe/H], Stars: Dwarfs, Stars: Late-Type

Scientific paper

In addition to Papers V and VI, this catalog draws on a review paper by the author on the SMR problem. If a star of interest for that problem appears without a value of [Fe/H] in Paper V, it is listed in the review paper and is also listed here with a designation "V." For all but two of these stars, mean values of [Fe/H] are given here. For the exceptions (HD 3765, HD 32147), low-resolution data suggest that [Fe/H] is substantially higher than published high-resolution results indicate (see the review paper). (2 data files).

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