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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 10080Å). 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 --------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 94 1143 Catalog of chromospheric emission lines
See also: J/A+A/439/1137 : PHOENIX model chromospheres of M dwarfs (Fuhrmeister+, 2005) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 8 F8.2 0.1nm lambda1 ? Measured wavelength 10- 14 F5.3 0.1nm FWHM ? Line FWHM 16- 23 E8.3 mW/m2 Flux ? Line flux 25- 33 F9.3 0.1nm lambda2 ? Cataloged wavelength 35- 38 A4 --- Ion Ion code 40- 43 I4 --- Mult ? Multiplet number 45 I1 --- IDflag Identification status flag (1) 47- 94 A48 --- Rem Remarks (2)
Note (1): Line identification status as follows: 0 = secure line identification 1 = probable line identification 2 = supplementary (weak) line (for completion of multiplet) 3 = poorly decomposed line, possibly additional lines existent 4 = no identification possible 5 = line measured in flare-only spectrum, secure identification 6 = line measured in flare-only spectrum, probable identification 7 = singlet line/single line from multiplet, but secure identification Note (2): Some abbreviations are used: n = line not measured in flare on LHS 2034 as found in J/A+A/439/1137 no gauss = line has no Gaussian shape, therefore flux poorly determined gauss affected = line in wing of non-Gaussian line: flux poorly determined NIST = identification from NIST catalog blend = gives alternative identification of line
Acknowledgements: Birgit Fuhrmeister, bfuhrmeister(at)hs.uni-hamburg.de
(End) Birgit Fuhrmeister [Uni. Hamburg], Patricia Vannier [CDS] 06-May-2008
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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