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J/A+A/326/1069      Abundances in globular clusters   (Russell 1997)

More Light on RV Tau Variables Russell S.C. <Astron. Astrophys. 326, 1069 (1997)> =1997A&A...326.1069R (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, globular ; Stars, giant ; Stars, variable ; Abundances Keywords: stars: abundances - stars: asymptotic, post-asymptotic giant branch (AGB, post-AGB) - stars: variables: other - globular clusters: general Description: Tables 5, 6, and 7 present details of the derived abundances for the stars observed in the globular clusters M2, M13, and M56, respectively. Table 9 gives the measured equivalent widths for the iron lines of the field stars. Table 10 gives the measured equivalent widths for the programme stars of this survey. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 21 33 29.2 -00 49 23 M 2 = NGC 7089 16 41 41.4 +36 27 37 M 13 = NGC 6205 19 16 35.4 +30 11 04 M 56 = NGC 6779 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table5 39 66 Measured Abundances for M2 table6 33 91 Measured Abundances for M13 table7 33 73 Measured Abundances for M56 table9 39 79 Equivalent widths for FeI and FeI for standard stars table10 85 309 Equivalent widths for programme stars tables.tex 117 701 LaTeX version of the tables
Byte-by-byte Description of file: table5
Bytes Format Units Label Explanations
1- 9 A9 --- Star Star Name 11- 15 A5 --- Element Element 17- 18 I2 --- Z Atomic Number 20- 23 F4.2 [] Solar Solar abundance (H=12) 25- 29 F5.2 [] Abundance ? Abundance of star 31- 34 F4.2 [] sigma ? Standard deviation of results 36- 37 I2 --- N ? number of lines used to derive abundance
Byte-by-byte Description of file: table6 table7
Bytes Format Units Label Explanations
1- 10 A10 --- Star Star Name 12- 16 A5 --- Element Element 18- 19 I2 --- Z Atomic Number 21- 25 F5.2 [] Abundance Abundance of star 27- 30 F4.2 [] sigma ? Standard deviation of results 32- 33 I2 --- N Number of lines used to derive abundance
Byte-by-byte Description of file: table9
Bytes Format Units Label Explanations
1- 5 A5 --- Element Element 7- 13 F7.2 0.1nm lambda Wavelength 15- 19 F5.1 0.1pm EW(HD165195) ? HD 165195 equivalent width 20 A1 --- u_EW(HD165195) Uncertainty flag on EW(HD165195) 22- 26 F5.1 0.1pm EW(BD+302611) ? BD +30 2611 equivalent width 28- 32 F5.1 0.1pm EW(HD204543) ? HD 204543 equivalent width 34- 38 F5.1 0.1pm EW(HD135148) ? HD 135148 equivalent width 39 A1 --- u_EW(HD135148) Uncertainty flag on EW(HD135148)
Byte-by-byte Description of file: table10
Bytes Format Units Label Explanations
1- 5 A5 --- Element Element 7- 8 I2 --- Z ? Atomic Number 10- 17 F8.3 0.1nm lambda Wavelength 19- 24 F6.3 --- loggf Oscillator strength 26- 29 A4 --- r_loggf Reference for loggf (1) 31- 35 F5.1 0.1pm EW(BD+112998) ? BD+11 2998 Equivalent width 36 A1 --- u_EW(BD+112998) Uncertainty flag on (BD+112998 38- 42 F5.1 0.1pm EW(M2V11) ? M2_V11 equivalent width 43 A1 --- u_EW(M2V11) Uncertainty flag on (M2V11) 45- 49 F5.1 0.1pm EW(M2HII89) ? M2HII89 equivalent width 50 A1 --- u_EW(M2HII89) Uncertainty flag on (M2HII89) 52- 56 F5.1 0.1pm EW(M13SH11) ? M13_SH11 equivalent width 57 A1 --- u_EW(M13SH11) Uncertainty flag on (M13SH11) 59- 63 F5.1 0.1pm EW(M13I13) ? M13I13 equivalent width 64 A1 --- u_EW(M13I13) Uncertainty flag on EW(M13I13) 66- 70 F5.1 0.1pm EW(M56V6) ? M56_V6 equivalent width 71 A1 --- u_EW(M56V6) Uncertainty flag on EW(M56V6) 73- 77 F5.1 0.1pm EW(M56I60) ? M56I60 equivalent width 78 A1 --- u_EW(M56I60) Uncertainty flag on EW(M56I60) 80- 84 F5.1 0.1pm EW(M56I96) ? M56I96 equivalent width 85 A1 --- u_EW(M56I96) Uncertainty flag on EW(M56I96)
Note (1): References: B92: Bessell M. S. 1992, private communication B,B+,C,C+,D,D-,E: accuracy ratings from NIST (1996) NIST Atomic Spectroscopic Database (Version 1.1) D+92: Davidson et al., 1992A&A...255..457D G+94: Giridhar et al., 1994ApJ...437..476G GS88: Gratton & Sneden, 1988A&A...204..193G H+82: Hannaford et al., 1982ApJ...261..736H K90: Kurucz, 1990, private communication PC89: Peterson & Carney, 1989ApJ...347..266P SC88: Sneden & Crocker, 1988ApJ...335..406S T89: Thevenin, 1989A&AS...77..137T T90: Thevenin, 1990A&AS...82..179T T94: Takeda, 1994PASJ...46...53T WM80: Wiese & Martin, 1980, NSRDS-NBS 60 (U.S. Government Printing Office, Washington, DC) WSM: Wiese, Smith, & Miles, 1969, Atomic Transition Probabilities, Vol 2, NSRDS-NBS 22 (U.S. Government Printing Office, Washington, DC)
Acknowledgements: Russell, S. C. [Dublin Institute for Advanced Studies]
(End) Patricia Bauer [CDS] 06-Jun-1997
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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