/ftp/cats/J/A%2BA/364/102



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J/A+A/364/102       Abundances of field BHB star candidates  (Kinman+, 2000)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	stars.dat table4.dat table5.dat
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Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=J/A+A/364/102
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drwxr-xr-x 12 cats archive 216 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 290 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 488 Dec 19 2022 .message -r--r--r-- 1 cats archive 5052 Dec 23 2000 ReadMe -rw-r--r-- 1 cats archive 320 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2527 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 709 Dec 22 2000 stars.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 5333 Dec 19 2000 table4.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 726 Dec 19 2000 table5.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/364/102 Abundances of field BHB star candidates (Kinman+, 2000) ================================================================================ A spectroscopic study of field BHB star candidates Kinman T., Castelli F., Cacciari C., Bragaglia A., Harmer D., Valdes F. <Astron. Astrophys. 364, 102 (2000)> =2000A&A...364..102K (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Stars, blue ; Abundances ; Equivalent widths Keywords: stars: abundances - stars: fundamental parameters - stars: horizontal-branch - stars: AGB and post-AGB - stars: white dwarfs - Galaxy: halo Abstract: New spectroscopic observations are presented for a sample of thirty-one blue horizontal branch (BHB) star candidates that are sufficiently nearby to have reliable proper motions. Comments are given on a further twenty-five stars that have previously been suggested as BHB star candidates but which were not included in our sample. Moderately high-resolution spectra (lambda/Deltalambda= 15000) of twenty five of our program stars were taken with the coude feed spectrograph at Kitt Peak. Twelve of the program stars were also observed with the CAT spectrograph at ESO. Six of these program stars were observed from both hemispheres. IUE low-resolution spectra are available for most of our candidates and were used, in addition to other methods, in the determination of their T_eff_ and reddening. Abundances were obtained from these spectra using models computed by Castelli with an updated version of the ATLAS9 code (Kurucz, 1993, CD-ROM No. 13). All thirty one candidates are halo stars.