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J/A+A/289/740       Galactic abundance gradients                 (Kaufer+, 1994)

The galactic abundance gradients traced by B-type stars KAUFER A., SZEIFERT T., KRENZIN R., BASCHEK B., WOLF B. <Astron. Astrophys. 289, 740 (1994)> =1994A&A...289..740K (SIMBAD/NED Reference)
ADC_Keywords: Stars, B-type; Spectroscopy; Abundances Keywords: stars: abundances, early type - Galaxy: abundances, evolution File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2 49 16 List of the stars table6 117 43 Measured equivalent width table7 117 109 Measured equivalent width table8 125 175 Measured equivalent width tables.tex 110 518 LaTeX version of tables 6, 7 and 8
Byte-by-byte Description of file: table2
Bytes Format Units Label Explanations
1- 11 A11 --- Name Object name 17 I1 --- Ref. Reference (1) 27- 31 F5.2 mag V visual magnitude 41- 44 F4.1 kpc Dgal galactocentric distance
Note (1): 1: Hoag A.A, Applequist N.L., 1965, ApJS 12, 215 2: Hiltner W.A., 1966, IAU Symp. 24, 373 3: Hoffleit D., Jaschek C., 1982, The Bright Star Catalogue, Yale University Observatory 4: Mermilliod J.C., 1986, Catalogue of UBV Photometry and MK Spectral Types in open clusters, Institute d'Astronomie de l'Universite de Lausanne 5: Moffat A.F.J., Vogt N., 1975, A&AS 20, 85
Byte-by-byte Description of file: table6
Bytes Format Units Label Explanations
1- 79 A79 --- Ident. Laboratory wavelengths of the contributing line components 82- 85 I4 0.1pm NGC6531/2 []? Measured equivalent width for NGC6531/2 90- 93 I4 0.1pm NGC6823/34 []? Measured equivalent width for NGC6823/34 98-101 I4 0.1pm NGC6910/2 []? Measured equivalent width for NGC6910/2 106-109 I4 0.1pm NGC1893/9 []? Measured equivalent width for NGC1893/9 114-117 I4 0.1pm NGC1893/10 []? Measured equivalent width for NGC1893/10
Byte-by-byte Description of file: table7
Bytes Format Units Label Explanations
1- 79 A79 --- Ident. Laboratory wavelengths of the contributing line components 82- 85 I4 0.1pm HR1763 []? Measured equivalent width for HR1763 90- 93 I4 0.1pm HR1765 []? Measured equivalent width for HR1765 98-101 I4 0.1pm HR1842 []? Measured equivalent width for HR1842 106-109 I4 0.1pm HR1886 []? Measured equivalent width for HR1886 114-117 I4 0.1pm HR1887 []? Measured equivalent width for HR1887
Byte-by-byte Description of file: table8
Bytes Format Units Label Explanations
1- 79 A79 --- Ident. Laboratory wavelengths of the contributing line components 82- 85 I4 0.1pm hPer/717 []? Measured equivalent width for hPer/717 90- 93 I4 0.1pm hPer/782 []? Measured equivalent width for hPer/782 98-101 I4 0.1pm S247/1 []? Measured equivalent width for S247/1 106-109 I4 0.1pm S301/3 []? Measured equivalent width for S301/3 114-117 I4 0.1pm S217/3 []? Measured equivalent width for S217/3 122-125 I4 0.1pm S208/6 []? Measured equivalent width for S208/6
Note: The equivalent widths of the metallic lines and non-diffuse He I lines were measured interactively by setting the continuum individually for each line and fitting a gaussian profile. The equivalent widths of the Balmer lines were measured interactively by removing strong blend components using a spline fit over the complete profile. This profile is finally integrated in fixed wavelength intervals of typically ±36 Angstroms (expect for S301/3 where the wavelength interval is ±30 Angstroms). The diffuse He I lines were measured in the same way.
(End) Patricia Bauer [CDS] 03-May-1994
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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