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J/AZh/79/841    Abundances of various elements in 20 Peg    (Rachkovskaya, 2002)

Abundances of carbon, nitrogen, oxygen, and other elements in the atmosphere of the giant 20 Peg Rachkovskaya T.M. <Astron. Zh. 79, 841 (2002)> =2002AZh....79..841R =2002ARep...46..760R
ADC_Keywords: Stars, giant; Spectroscopy ; Abundances, peculiar Abstract: Atmosphere study of the giant 20 Peg was investigated using high-resolution spectra. Description: The observations were acquired with the 2.6m reflector of the Crimean Astrophycal Observatory using an American-made EEV15-11 CCD array (1024x256 pixels) in September-October, 1995 and in January and October, 1999. Objects: ----------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------- 22 01 05.35 +13 07 11.4 20 Peg = HD 209166 ----------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 51 84 Lines studied in the spectrum of 20 Peg
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 4 A4 --- El Element name and ionisation 7- 13 F7.2 0.1nm Lambda Wavelength expressed in Angstroem 16- 20 F5.2 eV ExcPot Excitation potential of ground level 24- 28 F5.2 --- loggf1 Oscillator strength (log gf) from Vienna database (1) 31- 35 F5.2 --- loggf2 ? Oscillator strength (log gf) from previous work Rachkovskaya, 2000ARep...44..227R (2) 37- 39 I3 0.1nm EW Equivalent width 42- 45 F4.2 --- logeps1 Elemental abundance (H=12) based on Vienna database (1) 48- 51 F4.2 --- logeps2 ? Elemental abundance (H=12) based on Rachkovskaya, 2000ARep...44..227R (2)
Note (1): Vienna database was used : Piskunov et al., 1995A&AS..112..525P Note (2): Values from previous work, Rachkovskaya, 2000ARep...44..227R, was used

(End) Veta Avedisova (INASAN) 15-Feb-2003
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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