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J/A+A/354/899       Elemental abundance analyses IV.         (Adelman+, 2000)

Elemental abundance analyses with complejo astronomico El Leoncito REOSC echelle spectrograms. IV. Extensions of nine previous analyses. Adelman S.J., Pintado O.I. <Astron. Astrophys. 354, 899 (2000)> =2000A+A...354..899A
ADC_Keywords: Stars, peculiar ; Abundances, peculiar Keywords: stars: abundances - stars: chemically peculiar - Abstract: Using new CASLEO echelle spectrograms, we extended our elemental abundances of the sharp-lines Mercury-Manganese star µ Lep, 14 Hya, κ Cnc, HR 4487, 28 Her, and HR 7245, the closely related star 3 CenA, and 7 Sex an A0V star with population I abundances, but with Population II star space motion. The λλ4500-6200 region contains a sufficient number of lines to derive high-quality abundances of these stars. For most stars, the new spectra provide additional lines for the analyses which improve their quality as well as help fill in the periodic table. Description: Table 5 contains the Elemental Abundances From Newly Measured Lines. It is grouped by star and then subgrouped by atomic species with the lines listed by multiplet and within multiplets by numerical order. The columns are: multiplet number from Moore 1945, the wavelength in Angstroms, the log gf value, Ref. = Reference (two letter codes which are equivalenced to references at the end of the table), the equivalent width in mÅ, and the abundance relative to the total number of atoms per unit volume. For each atomic species the mean atomic species and the standard deviation of the mean (for 2 or more lines) are given. Entries are given only for newly measured lines. For additional lines please see earlier papers in this series. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 08 49 21.7 -03 26 35 14 Hya = HD 75333 = HR 3500 16 32 35.7 +05 31 16 28 Her = HD 149121 = HR 6158 13 51 49.6 -32 59 37 3 Cen A = HD 120709 = HR 5210 09 52 12.2 +02 27 15 7 Sex = HD 85504 = HR 3906 11 38 07.3 -61 49 36 HR 4487 = HD 101189 12 39 52.5 -39 59 14 HR 4817 = HD 110073 19 07 09.0 +00 38 28 HR 7245 = HD 178065 05 12 55.9 -16 12 20 mu Lep = HD 33904 = HR 1702 09 07 44.8 +10 40 05 kappa Cnc = HD 78316 = HR 3623 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file abund.dat 39 66 Atomic abundances table5.dat 54 651 Elemental abundances table5.tex 69 992 LaTeX version of table5.dat and abund.dat
See also: J/A+AS/125/219 : Paper II. (mu Lep, 7 Sex, HR 4817, 28 Her) (Adelman+ 1997) J/A+AS/129/563 : Paper III. (HR 4487, 14 Hyd and 3 Cen A) (Pintado+ 1998) J/A+AS/107/353 : CP stars (Lopez-Garcia+, 1994) J/A+AS/137/227 : HD 133029 & HD 192913 abundances (Lopez-Garcia+ 1999) J/MNRAS/316/514 : 28 And & 99 Her elemental abundances (Adelman+, 2000) 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: abund.dat
Bytes Format Units Label Explanations
1- 11 A11 --- Name Star name 14- 19 A6 --- Ion Ion 22- 24 I3 --- Nline Number of lines 26- 27 A2 --- Element Element (identical to bytes 14-15) 30- 34 F5.2 --- log(Nel/Ntot) Derived abundance of Element (ratio of number of atoms to the total number of atoms per unit volume) 36- 39 F4.2 --- e_log(Nel/Ntot) ? rms uncertainty on log(Nel/Ntot)
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 11 A11 --- Name Star name 13- 18 A6 --- Ion Ion 20- 26 A7 --- Mult ? Multiplet number 28- 34 F7.2 0.1nm lambda Wavelength 36- 40 F5.2 --- log(gf) Oscillator strength 43- 44 A2 --- r_log(gf) Reference for log(gf) (1) 46- 48 I3 10-4nm EW ? Equivalent width 50- 54 F5.2 --- log(N/Ntot) Derived abundance in relative number of atoms per unit volume
Note (1): the references are: FW = Fuhr & Wiese (1990, in Lide, D. R. ed, CRC Handbook of Chemistry and Physics, CRC Press, Cleveland, OH) HL = Hannaford et al. (1982ApJ...261..736H) KX : Kurucz, 1995, in Astrophysical Applications of Powerful New Databases, eds. S. J. Adelman and W. L. Wiese (ASP, San Francisco), ASP Conf. Ser. 78, 205 MF : Martin et al., 1988, and Fuhr et al. 1988, Cat. VI/72 WF : Wiese et al., 1996, J. Phys. Chem. Ref. Data, Monograph 6 WM = Wiese & Martin, 1980, NSRDS-NBS 68. Part 2, US Government Printing Office, Washington, DC. WS : Wiese et al., 1966, NSRDS-NBS 4, US Government Printing, Office, Washington, DC and 1969, NSRDS-NBS, Washington, D.C., US Department of Commerce, National Bureau of Standards
Acknowledgements: Saul J. Adelman References: Pintado & Adelman, Paper I. (kappa Cnc, HR 7245, ξ Oct) 1996A&AS..118..283P
(End) Patricia Bauer [CDS] 13-Jan-2000
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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