Emission lines in a giant flare of CN Leo (Fuhrmeister+, 2008)

Details Emission lines in a giant flare of CN Leo (Fuhrmeister+, 2008) Emission lines in a giant flare of CN Leo (Fuhrmeister+, 2008)

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34870293f&link_type=abstract

VizieR On-line Data Catalog: J/A+A/487/293. Originally published in: 2008A&A...487..293F

Physics

Stars: Late-Type, Stars: M-Type

Scientific paper

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 10080{AA}). 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.
(1 data file).

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