========================================================================== J/A+AS/146/437 IR spectra of oxygen-rich evolved stars (Speck+, 2000) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table1.dat table2.dat table3.dat table4.dat table5.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=J/A+AS/146/437 ==========================================================================
drwxr-xr-x 13 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:56 [TAR file] -rw-r--r-- 1 cats archive 509 Nov 19 2000 .message -r--r--r-- 1 cats archive 5299 Nov 19 2000 ReadMe -rw-r--r-- 1 cats archive 446 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 3442 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 9837 Nov 17 2000 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 5552 Dec 12 2000 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -rw-r--r-- 1 cats archive 1809 Nov 19 2000 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1098 Dec 12 2000 table4.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1896 Nov 19 2000 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+AS/146/437 IR spectra of oxygen-rich evolved stars (Speck+, 2000) ================================================================================ Dust features in the 10-mum infrared spectra of oxygen-rich evolved stars. Speck A.K., Barlow M.J., Sylvester R.J., Hofmeister A.M. <Astron. Astrophys. Suppl. Ser. 146, 437 (2000)> =2000A&AS..146..437S ================================================================================ ADC_Keywords: Stars, supergiant ; Spectra, infrared Keywords: (stars:) circumstellar matter - stars: mass-loss - stars: AGB and post-AGB - (stars:) supergiants - infrared: stars - stars: variables: other Abstract: We have analyzed the 8-13.5mum UKIRT CGS3 spectra of 142 M-type stars including 80 oxygen-rich AGB stars and 62 red supergiants, with a view to understanding the differences and similarities between the dust features of these stars. We have classified the spectra into groups according to the observed appearance of the infrared features.
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