/ftp/cats/ii/66



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II/66           A Catalogue of observations in H alpha    (Ducati, 1981)
The following files can be converted to FITS (extension .fit .fiz or .fiZ)
	obs.dat means.dat refs.dat
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Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=II/66
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drwxr-xr-x 351 cats archive 8192 Mar 25 10:13 [Up] drwxr-xr-x 2 cats archive 4096 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 471 Dec 19 2022 .message -r--r--r-- 1 cats archive 5010 Jun 18 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 48279 May 12 1997 means.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 274365 May 12 1997 obs.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2329 May 12 1997 refs.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : II/66 A Catalogue of observations in H alpha (Ducati, 1981) ================================================================================ A Catalogue of observations in H alpha Ducati J.R. <Astron. Astroph. Suppl. 45, 119, (1981)> =1981A&AS...45..119D ================================================================================ ADC_Keywords: Photometry, H-alpha ; Equivalent widths Abstract: This catalogue contains 4095 published observations of the quantitative observations of Halpha for 2700 stars. These observations were collected from values published between 1949 and 1980. The Halpha index was reduced to a common system described by Strauss & Ducati (1981A&AS...44..337S); the values of the original index can be retrieved with a linear transformation (cc = correlation coefficient): ----------------------------------------------------------------- References a b cc lower upper Spectral range ----------------------------------------------------------------- 2 1.401 -1.604 0.972 1.050 1.170 10 1.33 -2.4 0.000 13 1.526 0.130 0.992 2.910 3.300 14,36 0.343 0.814 0.949 1.400 O B A0 14,36 0.269 0.969 0.972 1.470 A1 F G K M 20,21,22,23,37 0.39 -0.55 1.200 24,25 1.35 -1.48 0.922 1.020 1.170 -----------------------------------------------------------------