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J/PASJ/58/389    O/Fe abundances of 15 RR Lyrae              (Takeda+, 2006)

On the spectroscopic determination of atmospheric parameters and O/Fe abundances of RR Lyrae stars. Takeda Y., Honda S., Aoki W., Takada-hidai M., Zhao G., Chen Y.-Q., Shi J.-R. <Publ. Astron. Soc. Jap., 58, 389-406 (2006)> =2006PASJ...58..389T
ADC_Keywords: Stars, variable ; Abundances, peculiar ; Stars, atmospheres Keywords: stars: abundances - stars: atmospheres - stars: fundamental parameters - stars: individual (RR Lyr, DX Del, DH Peg, VY Ser) - stars: variables: other Abstract: In order to study how the conventional spectroscopic method based on the equivalent widths of the Fe I and Fe II lines effectively applies to determining the atmospheric parameters (Teff, logg, vt, [Fe/H]) of RR Lyrae variables and how accurately the abundances can be established from such constructed model atmospheres, we analyzed 15 high-dispersion spectrograms of RR Lyr, DX Del, DH Peg, and VY Ser taken at several different phases by using the HDS spectrograph of the Subaru Telescope, and examined the consistency of the resulting phase-to-phase abundances. Description: The file, ewidlist.dat, in which the equivalent widths data of the Fe I and Fe II lines measured from each of the 15 spectra for four stars (RR Lyr, DX Del, DH Peg, and VY Ser) are presented. Here, all measured data are given irrespective of whether or not they were actually used for the parameter determination. (Regarding the finally adopted lines for parameter determinations which remained after the rejection process of some inappropriate lines, see other tables.) Other files, each corresponding to each of the 15 spectra for four stars (RR Lyr, DX Del, DH Peg, and VY Ser), contain the adopted data of equivalent widths and the abundance results of the Fe I and Fe II lines corresponding to the finally converged solutions of the atmospheric parameters. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 19 25 27.9 +42 47 04 RR Lyr = HD 182989 20 47 28.4 +12 27 51 DX Del = BD+11 4381 22 15 25.6 +06 49 21 DH Peg = BD+06 4990 15 31 01.9 +01 41 02 VY Ser = HD 138279 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file ewidlist.dat 139 220 Fe line data and the measured equivalent widths tabe2/* 55 16 EW data for TT Lyr, DX Del, DH Peg, VY Ser and Sun
Description of file: ewidlist.dat The data contained in this file are divided into two parts: atomic data of 220 Fe I/II lines and their equivalent widths measured on each of the 15 spectra of RR Lyr, DX Del, DH Peg, and VY Ser. All the atomic data were taken from the compilation of Kurucz and Bell (1995, Kurucz CD-ROM, No. 23 ). The meanings of these line data are mostly self-explanatory. Regarding the definition of the damping parameters (gammar, gammas, gammas) adopted here, see, for example, the caption in table 1 of Takeda (2003, Cat. J/A+A/402/343). When the equivalent widths were not (could not be) measured, zero values are assigned. Description of files: tabe2/*: The 7 characters "???????" of the file name indicates the spectrum label. The first four lines are the header part which includes the information concerning the final parameter solutions. !!!!!!! Remark: The quantity "xcur" in the first line is the differential metallicity (relative to the Sun) formally evaluated as A(Fe)-7.50. However, since we adopted A(Fe:Sun) = 7.60 as the standard solar abundance (cf. subsection 3.1), our final [Fe/H] is eventually related to this xcur as [Fe/H] = xcur - 0.1. !!!!!!! From the 5th line begins the actual data for each of the used Fe lines: line number, species code, wavelength, lower excitation potential, gf value, measured equivalent width, and the resulting Fe abundance corresponding to the final solution of Teff, log g, and vt. The Fe abundances are repeatedly listed twice in columns 7 and 8 with different signs for neutral and ionized species, such as [+A(FeI),-A(FeII)] in column 7 and [-A(FeI),+A(FeII)] in column 8, in order for the convenience of plotting the FeI and FeII data with different symbols. See also: J/A+A/308/481 : Metallic line doubling phenomenon in RR Lyrae (Chadid+, 1996) Byte-by-byte Description of file: ewidlist.dat
Bytes Format Units Label Explanations
1- 4 I4 --- Line Line number (7000- for Fe I 8000- for Fe II) 5- 10 F6.2 --- Code Species code (26.00: Fe I, 26.01: Fe II) 11- 19 F9.3 0.1nm Lambda Wavelength 20- 25 F6.2 eV Ep Lower excitation potential 26- 31 F6.2 --- loggf log gf value 32- 37 F6.2 --- Gammar Radiation damping parameter 38- 43 F6.2 --- Gammas Quadratic Stark effect damping parameter 44- 49 F6.2 --- Gammaw van der Waals effect damping parameter 50- 55 F6.1 0.1pm EW(rrlyr1) ?=0.0 Equivalent width for spectrum rrlyr-1 56- 61 F6.1 0.1pm EW(rrlyr2) ?=0.0 Equivalent width for spectrum rrlyr-2 62- 67 F6.1 0.1pm EW(rrlyr3) ?=0.0 Equivalent width for spectrum rrlyr-3 68- 73 F6.1 0.1pm EW(rrlyr4) ?=0.0 Equivalent width for spectrum rrlyr-4 74- 79 F6.1 0.1pm EW(rrlyr5) ?=0.0 Equivalent width for spectrum rrlyr-5 80- 85 F6.1 0.1pm EW(dxdel1) ?=0.0 Equivalent width for spectrum dxdel-1 86- 91 F6.1 0.1pm EW(dxdel2) ?=0.0 Equivalent width for spectrum dxdel-2 92- 97 F6.1 0.1pm EW(dxdel3) ?=0.0 Equivalent width for spectrum dxdel-3 98-103 F6.1 0.1pm EW(dhpeg1) ?=0.0 Equivalent width for spectrum dhpeg-1 104-109 F6.1 0.1pm EW(dhpeg2) ?=0.0 Equivalent width for spectrum dhpeg-2 110-115 F6.1 0.1pm EW(dhpeg3) ?=0.0 Equivalent width for spectrum dhpeg-3 116-121 F6.1 0.1pm EW(vyser1) ?=0.0 Equivalent width for spectrum vyser-1 122-127 F6.1 0.1pm EW(vyser2) ?=0.0 Equivalent width for spectrum vyser-2 128-133 F6.1 0.1pm EW(vyser3) ?=0.0 Equivalent width for spectrum vyser-3 134-139 F6.1 0.1pm EW(vyser4) ?=0.0 Equivalent width for spectrum vyser-4
Byte-by-byte Description of file (# headlines): tabe2/*
Bytes Format Units Label Explanations
1- 4 I4 --- Line Line number 5- 10 F6.2 --- Code FeI: 26.00 FeII: 26.01 11- 19 F9.3 0.1nm Lambda Wavelength 20- 26 F7.3 eV Ep Lower excitation potential (chi) 27- 33 F7.3 --- loggf Adopted log(gf) value 34- 39 F6.1 0.1pm EW Equivalent width 40- 47 F8.3 --- Abund1 Fe abundance (sign inversed for Fe II lines) 48- 55 F8.3 --- Abund2 Fe abundance (sign inversed for Fe I lines)
Acknowledgements: Maho Kuroiwa, maho(at)pasj.asj.or.jp
(End) Patricia Vannier [CDS] 16-May-2006
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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