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J/A+A/381/507       Fe II emission lines of RR Tel        (Kotnik-Karuza+, 2002)

The region of Fe II emission line formation of the symbiotic nova RR Tel. Kotnik-Karuza D., Friedjung M., Selvelli P.L. <Astron. Astrophys. 381, 507 (2002)> =2002A&A...381..507K
ADC_Keywords: Stars, variable ; Novae ; Spectroscopy Keywords: stars: binaries: symbiotic - stars: individual: RR Tel - stars: fundamental parameters Description: Files table1.dat and table2.dat contain the permitted and forbidden Fe II emission lines respectively which have been selected from the optical spectrum of RR Tel between 3180 and 9455Å. The spectrum was observed by Crawford et al. (1999, Cat. J/A+AS/139/135) whose corrected line fluxes and velocity widths we took for further analysis in this work. In the tables there are also values characteristic for the corresponding multiplets and lines such as multiplet numbers, term designations, level excitation potentials and quantum numbers J. The log functions of gf's, line fluxes and wavelengths are relevant for the SAC curves. Objects: ----------------------------------------- RA (2000) DE Designation(s) ----------------------------------------- 20 04 19.0 -55 43 30 RR Tel ----------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 89 82 *Accepted permitted Fe II lines from the identification list of Crawford (Crawford et al., 1999, Cat. J/A+AS/139/135) which have been analysed in this work by the SAC method table2.dat 97 49 *Accepted forbidden Fe II lines from the identification list of Crawford (Crawford et al., 1999, Cat. J/A+AS/139/135) which have been analysed in this work by the SAC method
Note on table1.dat and table2.dat: Friedjung-Muratorio self absorption curve (SAC) method (Friedjung & Muratorio, 1987A&A...188..100F)
See also: J/A+AS/139/135 : The Optical Spectrum of RR Tel (Crawford+ 1999) Byte-by-byte Description of file: table1.dat table2.dat
Bytes Format Units Label Explanations
1- 5 F5.3 10-12mW/m2 Intc Corrected intensity 7- 13 F7.2 0.1nm Lambda Laboratory wavelength 15- 16 I2 --- Mult Multiplet number 18- 23 F6.3 --- log(gf) Oscillator strength 25- 29 F5.2 --- log(Fl3/gf) Normalized flux defined by the SAC method (Friedjung & Muratorio, 1987A&A...188..100F) 31- 35 F5.2 --- log(gfl) Lower term oscillator strength 37- 38 I2 km/s FWHM Velocity FWHM 40- 42 A3 --- l Lower term of the multiplet 44- 47 A4 --- u Upper term of the multiplet 49- 52 F4.2 eV EPl Excitation potential of the lower level 54- 57 F4.2 eV EPu Excitation potential of the upper level 59- 63 A5 --- Ju J number of the upper level
Acknowledgements: Dubravka Karuza
(End) Patricia Bauer [CDS] 09-Nov-2001
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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