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J/A+A/507/881       Emission lines in EX Lup optical spectrum     (Sipos+, 2009)

EX Lupi in quiescence. Sipos N., Abraham P., Acosta-Pulido J., Juhasz A., Kospal A., Kun M., Moor A., Setiawan J. <Astron. Astrophys. 507, 881 (2009)> =2009A&A...507..881S
ADC_Keywords: Stars, pre-main sequence ; Spectroscopy ; Equivalent widths Keywords: stars: formation - stars: circumstellar matter - stars: individual: EX Lup - stars: infrared Abstract: A high-resolution optical spectrum of EX Lupi was obtained on 2007 July 30 with FEROS at the 2.2m MPG/ESO telescope in ESO La Silla, Chile. The spectrum shows several emission lines in addition to the photospheric absorption features characteristic of the young late-type star. Here we present all emission lines identified in the spectrum, the observed wavelengths and equivalent widths in Angstrom and the full widths at half maximum in km/s, determined by Gaussian fitting. The most prominent emission lines are the Balmer lines of the hydrogen, the H and K lines and the infrared triplet of the ionized calcium, and the helium lines at 5875 and 6678 Angstrom, and in addition more than 200 weak, narrow metallic lines could be identified using Moore's (1945, Contrib. Princeton Univ. Obs., No. 20) multiplet tables. Objects: ------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------ 16 03 05.5 -40 18 25 EX Lup = HD 325367 ------------------------------------------------ File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file exlupisp.dat 62 194 Emission lines identified in the optical spectrum of EX Lupi (table3 of the paper)
Byte-by-byte Description of file: exlupisp.dat
Bytes Format Units Label Explanations
1- 7 F7.2 0.1nm lambda Wavelength 12- 17 F6.2 0.1nm EW Equivalent width (negative for absorption) 21- 26 F6.2 km/s FWHM Full width at half maximum determined Gaussian fitting 29- 62 A34 --- Line Observed emission line(s) with multiplet number
Acknowledgements: Nikoletta Sipos, niki(at)
(End) N. Sipos [Konkoly Observatory, Hungary], P. Vannier [CDS] 29-Oct-2009
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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