========================================================================== J/A+A/416/281 X-ray spectra of 4 cool stars (Sanz-forcada+, 2004) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table?.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/416/281 ==========================================================================
drwxr-xr-x 19 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Jun 16 11:04 [TAR file] -rw-r--r-- 1 cats archive 469 May 2 2004 .message -r--r--r-- 1 cats archive 4463 May 2 2004 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 7354 Mar 1 2004 table4.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 6240 Mar 1 2004 table5.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 7911 Mar 1 2004 table6.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3582 Mar 1 2004 table7.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 28873 Mar 1 2004 tables.ps.gz [Uncompressed] -r--r--r-- 1 cats archive 40246 Mar 1 2004 tables.tex
Beginning of ReadMe : J/A+A/416/281 X-ray spectra of 4 cool stars (Sanz-forcada+, 2004) ================================================================================ Coronal versus photospheric abundances of stars with different activity levels. Sanz-forcada J., Favata F., Micela G. <Astron. Astrophys., 416, 281-290 (2004)> =2004A&A...416..281S ================================================================================ ADC_Keywords: Stars, late-type ; X-ray sources ; Spectroscopy Keywords: stars: coronae - stars: abundances - stars: late-type - X-rays: stars - line: identification Description: These tables include the observed fluxes of the lines identified in the X-ray spectra of four cool stars (Procyon, epsilon Eri, lambda And and V851 Cen). The spectra were taken using different configurations (Chandra/LETG, Chandra/HETG and XMM/RGS). The tables list the observed fluxes at Earth, and a comparison with the fluxes predicted for a given thermal coronal structure (the Emission Measure Distribution, EMD), the emissivities provided by the Astrophysical Plasma Emission Model (APED) and column density of absorbing material in the interstellar medium towards the star. A list of the most important (at least a 5% of the flux predicted for the line) blends that have been considered for each line is included. Objects: --------------------------------------------------------------------- RA (2000) DE Designation(s) (File) --------------------------------------------------------------------- 03 32 55.8442 -09 27 29.744 epsilon Eri = HD 22049 (table5.dat) 07 39 18.1183 +05 13 29.975 Procyon = HD 61421 (table4.dat) 13 44 00.9239 -61 21 59.148 V851 Cen = HD 119285 (table7.dat) 23 37 33.8425 +46 27 29.347 lambda And = HD 222107 (table6.dat) ---------------------------------------------------------------------
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