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J/A+AS/111/17       Abundance analysis of stars in NGC 6522      (Castro+, 1995)

High-resolution abundance analysis of two stars near the globular cluster NGC 6522 projected in Baade's window. CASTRO S., BARBUY B., BICA E., ORTOLANI S., RENZINI A. <Astron. Astrophys. Suppl. Ser. 111, 17 (1995)> =1995A&AS..111...17C (SIMBAD/NED Reference)
ADC_Keywords: Clusters, globular; Spectroscopy; Abundances Keywords: bulge - globular clusters - abundances Description: The CASPEC echelle spectrograph at the ESO 3.6 m telescope was used to obtain high resolution spectra of Arp 1145 and Arp 2240, two stars of the Baade Window, near the globular cluster NGC 6522. From a detailed analysis using equivalent widths and spectrum synthesis we derive the stellar parameters (Teff, log g and [M/H])=(4750,1.2,-0.9) and (5000,2.15,+0.2), respectively for Arp 1145 and Arp 2240. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table 57 254 Equivalent widths of Arp 1145 and Arp 2240
Byte-by-byte Description of file: table
Bytes Format Units Label Explanations
3- 10 F8.3 0.1nm Lambda Wavelength 17- 18 A2 --- El Element 19 I1 --- Ioniz Ionization stage 26- 29 F4.2 eV ExcPot Excitation potential 33- 37 F5.2 --- loggf Oscillator strength (log gf) 44- 47 F4.0 0.1pm WArp1145 []? Equivalent widths for Arp1145 52- 55 F4.0 0.1pm WArp2240 []? Equivalent widths for Arp2240

(End) Patricia Bauer [CDS] 20-Dec-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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