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J/A+AS/137/227   HD 133029 & HD 192913 elemental abundances (Lopez-Garcia+ 1999)

Elemental abundance studies of CP stars. II. The silicon stars HD 133029 and HD 192913 Lopez-Garica Z., Adelman S.J. <Astron. Astrophys. Suppl. Ser. 137, 227 (1999)> =1999A&AS..137..227L (SIMBAD/NED BibCode)
ADC_Keywords: Stars, peculiar ; Abundances, peculiar ; Equivalent widths Keywords: stars: chemically peculiar - stars: abundances - stars: individual: HD 133029 - stars: individual: HD 192913 Abstract: Fine analyses of the silicon stars HD 133029 and HD 192913 are presented using ATLAS9 model atmospheres whose predictions fit the optical region spectrophotometry and Hγ profiles and have the same bulk metallicity as the deduced abundances. Both are very He poor stars. The light elements are mostly solar except for silicon, and all the heavier elements, except nickel in HD 133029 which is solar, are greatly overabundant. The iron peak elements are typically 10 times overabundant. SrYZr are of order of 100 times solar. The rare earths are 1000 or more times overabundant. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 15 00 38.7 +47 16 39 HD 133029 20 16 27.2 +27 46 34 HD 192913 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4a.dat 48 433 Elemental abundances table4b.dat 28 29 Relative abundances table4.tex 123 672 LaTeX version of table4
See also: J/A+AS/107/353 : Paper I. HD 43819, HD 147550 (Lopez-Garcia+, 1994) J/A+A/367/859 : Paper III. α Scl and HD 170973 (Lopez-Garcia+, 2001) J/A+AS/125/219 : mu Lep, 7 Sex, HR 4817 & 28 Her abundances (Adelman+ 1997) J/A+AS/129/563 : Abundances of HR 4487, 14 Hyd and 3 Cen A (Pintado+ 1998) J/A+A/354/899 : Elemental abundance analyses. IV. (Adelman+, 2000) J/MNRAS/316/514 : 28 And & 99 Her elemental abundances (Adelman+, 2000) J/A+A/367/597 : ups Her, phi Her & HR 7018 abundances (Adelman+, 2001) J/A+A/394/187 : γ Ser & 101 Her elemental abundances (Caliskan+, 2002) J/A+A/406/975 : theta And, eps Del, eps Aqr, iota And (Kocer+, 2003) J/A+A/406/987 : xi Oct, alpha Sex, 68 Tau elemental abund. (Pintado+, 2003) Byte-by-byte Description of file: table4a.dat
Bytes Format Units Label Explanations
1- 6 A6 --- El Element 8- 10 I3 --- No ? Multiplet Number 12- 19 F8.3 0.1nm Lambda Wavelength 21- 25 F5.2 --- log(gf) Oscillator strength 27- 28 A2 --- r_log(gf) Reference to oscillator strength (1) 30- 32 I3 0.1pm W1 ? Equivalent width for HD 133029 34- 38 F5.2 --- log(N/Ntot)1 ? Deduced abundance for HD 133029 (2) 40- 42 I3 0.1pm W2 ? Equivalent width for HD 192913 44- 48 F5.2 --- log(N/Ntot)2 ? Deduced abundance for HD 192913 (2)
Note (1): Sources of gf-values: BG = Biemont et al. (1981ApJ...248..867B) BK = Biemont et al. (1982A&A...107..166B) DW = Dworetsky (1980A&A....84..350D) GB = Grevesse et al. (1981, Upper Main Sequence CP Stars, 23rd. Liege Astrophys. Coll., 211) HL = Hannaford et al. (1982ApJ...261..736H) KX = Kurucz (1992RMxAA..23...45K) LA = Lanz & Artru (1985PhyS...32..115L) MC = Magazzu & Cowley (1986ApJ...308..254M) MF = Martin, Fuhr & Wiese (1988, Cat. VI/72) for Sc through Mn; Fuhr, Martin & Wiese (1988, Cat. VI/72) for Fe through Ni; SC = Schaeffer (1971ApJ...163..411S) WD = Ward (1985MNRAS.213...71W) WF = Wiese & Fuhr (1975JPCRD...4..263W) WM = Wiese & Martin (1980, NSRDS-NBS 68, Part.2, US Governement Printing Office, Washington) WS= Wiese, Smith & Glennon (1966, NSRDS-NBS 4, US Governement Printing Office, Washington) and Wiese, Smith & Miles (1969, NSRDS-NBS, D.C.: US Department of Commerce, National Bureau of Standards) Note (2): N = number of atoms/volume of particular element Ntotal = number of atoms/volume of all elements
Byte-by-byte Description of file: table4b.dat
Bytes Format Units Label Explanations
1- 6 A6 --- El Element 8- 12 F5.2 --- log(El/Ntot)1 ? Elemental abundance for HD 133029 (1) 14- 17 F4.2 --- e_log(El/Ntot)1 ? rms uncertainty on log(El/Ntot)1 19- 23 F5.2 --- log(El/Ntot)2 ? Elemental abundance for HD 192913 (1) 25- 28 F4.2 --- e_log(El/Ntot)2 ? rms uncertainty on log(El/Ntot)2
Note (1): El = Element Ntot = number of atoms/volume of all elements
Acknowledgements: Saul J. Adelman
(End) Patricia Bauer [CDS] 19-Feb-1999
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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