J/BaltA/21/219        Spectroscopy of ups Sgr              (Kipper+, 2012)

High-resolution spectroscopy of the hydrogen-deficient binary υ Sgr. Kipper T., Klochkova V.G. <Baltic Astron., 21, 219-240 (2012)> =2012BaltA..21..219
ADC_Keywords: Stars, Be ; Stars, atmospheres ; Abundances Keywords: stars: atmospheres - stars: individual: upsilon Sgr Abstract: The high resolution spectra of hydrogen-deficient binary υ Sgr are analyzed. The atmospheric parameters are Teff= 12300±200K, logg=2.5±0.5 and ξt=5-15km/s depending on the element. Description: Our high resolution spectra (R=45000) were obtained with the Nasmyth Echelle Spectrograph NES permanently located at the Nasmyth focus of the 6 meter telescope of the Special Astrophysical Observatory. Objects: --------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------- 19 21 43.62 -15 57 18.1 ups Sgr = HD 181615 --------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 76 62 The lines with P Cygni profiles in the spectrum of υ Sgr table7.dat 38 667 Atomic data for υ Sgr -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 F8.3 0.1nm lam.a Absorption line wavelength 10- 13 F4.1 km/s RV.a Radial velocity for absorption line 15- 18 F4.1 pm EW.a Equivalent width for absorption line 20- 27 F8.3 0.1nm lam.R Red line wavelength 29- 32 F4.1 km/s RV.R Radial velocity for red line 34- 37 F4.1 pm EW.R Equivalent width for red line 39- 46 F8.3 0.1nm lam.B ? Blue line wavelength 48- 52 F5.1 km/s RV.B ? Radial velocity for blue line 54- 56 F3.1 pm EW.B ? Equivalent width for blue line 58- 61 A4 --- El Identification for element 63- 70 F8.3 0.1nm lam.el Identification for wavelength 72- 76 F5.2 [-] eps(low) Lower value for abundance logε (H=12) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- El Element 8- 15 F8.2 0.1nm lambda Wavelength 17- 21 F5.2 eV EPi Lower level excitation potential 23- 27 F5.2 [-] loggf Oscillator strength 29- 32 F4.1 pm EW Equivalent width 34- 38 F5.2 [-] logeps Abundance (calculated assuming Teff=12000K, logg=2.5) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 24-Dec-2012
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