========================================================================== J/A+A/487/293 CN Leo giant flare emission lines (Fuhrmeister+, 2008) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table1.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/487/293 ==========================================================================
drwxr-xr-x 20 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:57 [TAR file] -rw-r--r-- 1 cats archive 469 Sep 21 2008 .message -r--r--r-- 1 cats archive 4415 Sep 21 2008 ReadMe -r--r--r-- 1 cats archive 56900 May 6 2008 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/487/293 Emission lines in a giant flare of CN Leo (Fuhrmeister+, 2008) ================================================================================ Multi-wavelength observations of a giant flare on CN Leonis I. Fuhrmeister B., Liefke C., Schmitt J.H.M.M., Reiners A. <Astron. Astrophys. 487, 293 (2008)> =2008A&A...487..293F ================================================================================ ADC_Keywords: Stars, late-type; Stars, M-type Keywords: stars: activity - stars: flare - stars: chromospheres - stars: late-type - stars: individual: CN Leo Abstract: Flares on dM stars contain plasmas at very different temperatures and thus affect a wide wavelength range in the electromagnetic spectrum. While the coronal properties of flares are studied best in X-rays, the chromosphere of the star is observed best in the optical and ultraviolet ranges. Therefore, multiwavelength observations are essential to study flare properties throughout the atmosphere of a star. Description: We present an extensive identification catalog of chromospheric emission lines in the optical range for a giant flare on CN Leonis. The data were obtained with ESO's Kueyen telescope equipped with the UVES spectrograph on May, 19th/20th, 2006. The instrument was operated in dichroic mode (spectral coverage from 3050 to 3860 and from 6400 to 10080AA). We tabulate measured wavelength, line flux and FWHM for every line and also provide the rest wavelength from the Moore catalog which was used for identification (Moore, 1972, Nat. Stand. Ref. Data. Ser., 40). Few lines were identified with the NIST database. Objects: --------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------- 10 56 28.9 +07 00 53 CN Leo = Wolf 359 ---------------------------------------------
© UDS/CNRS