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J/PAZh/26/465   IRAS 20004+2955 (V1027 Cyg) chemical comp.   (Klochkova+, 2000)

Optical spectrum of the infrared source IRAS 20004+2955 (V1027 Cyg). Klochkova V.G., Mishenina T.V., Panchuk V.E. <Pis'ma Astron. Zh. 26, 465 (2000)> =2000PAZh...26..465K =2000AstL...26..398K
ADC_Keywords: Stars, variable; Equivalent widths; Abundances Abstract: Based on high-dispersion echelle spectra taken with the 6-m telescope, detailed chemical composition of the IR source IRAS 20004+2955 identified with the variable star V1027 Cyg is studied. Object: ------------------------------------------------------------------------- RA (2000) DE Designation ------------------------------------------------------------------------- 20 02 27.38 +30 04 25.5 V1027 Cyg = IRAS 20004+2955 = HD 333385 ------------------------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 47 115 Atomic data, equivalent widths of special lines and elemental abundances for two atmosphere models table3.dat 37 19 Atmospheric elemental abundances for V1027 Cyg
See also: J/PAZh/26/510 : Spectrum of bipolar nebula AFGL 2688 (Klochkova+, 2000) J/PAZh/26/115 : Spectrum of IRAS 23304+6147 (Klochkova+, 2000) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 4 A4 --- El Element 7- 14 F8.3 0.1nm Lambda Wavelength 17- 20 F4.2 eV ExcPot Excitation potentials of the lower level 23- 27 F5.2 --- Loggf Oscillator strength (log gf) 30- 35 F6.2 0.1um EW Equivalent width 38- 41 F4.2 --- A(X)1 Chemical composition for the model: Teff=5000K, logg=1.0 44- 47 F4.2 --- A(X)2 Chemical composition for the model: Teff=4900K, logg=0.5;
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 4 A4 --- El Element 6- 7 I2 --- n Number of the lines used 10- 13 F4.2 --- logA1 Mean atmospheric elemental abundances for Teff=5000K, logg=1.0 16- 19 F4.2 --- e_logA1 ? rms uncertainty on logA1 22- 25 F4.2 --- logA2 Mean atmospheric elemental abundance for Teff=4900K, logg=0.5 28- 31 F4.2 --- e_logA2 ? rms uncertainty on logA2 34- 37 F4.2 --- logASun Solar atmospheric elemental abundance

(End) Veta Avedisova [INASAN] 29-Jun-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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