/ftp/cats/V/88



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V/88                 Averaged [Fe/H] for Cool Dwarfs       (Taylor, 1995)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	fehd.dat refs.dat
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Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=V/88
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drwxr-xr-x 136 cats archive 4096 Jul 11 12:05 [Up] drwxr-xr-x 2 cats archive 4096 Dec 15 2013 [TAR file] -rw-r--r-- 1 cats archive 460 Jun 5 1998 .message -r--r--r-- 1 cats archive 5145 May 20 1998 ReadMe -rw-r--r-- 1 cats archive 213 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 23035 May 20 1998 fehd.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 12628 Jul 13 1995 program.for -r--r--r-- 1 cats archive 7460 Jul 13 1995 refs.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : V/88 Averaged [Fe/H] for Cool Dwarfs (Taylor, 1995) ================================================================================ Analyses of Archival Data for Cool Dwarfs. V. an Annotated Catalog of Averaged Values of [Fe/H] Taylor B.J. <PASP, 106, 704 (1994)> =1994PASP..106..704T Analyses of Archival Data for Cool Dwarfs. VI. The 1993 Versions of the Temperature and [Fe/H] Catalogs Taylor B.J. <PASP, 107, 734 (1995)> =1995PASP..107..734T ================================================================================ ADC_Keywords: Abundances, [Fe/H]; Stars, dwarfs; Stars, late-type Abstract: This file contains mean values of [Fe/H] (with rms errors) for 495 F-K stars which are on or near the main sequence. Literature references are given for the contributing values of [Fe/H]. Introduction: 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).

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