J/A+A/326/1069 J/A+A/326/1069 Abundances in globular clusters S C Russell Astron. Astrophys. 326 1069 1997 1997A&A...326.1069R Abundances Clusters, globular Stars, giant Stars, variable globular clusters: general stars: abundances stars: AGB and post-AGB stars: variables: other 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.

M 2NGC 708921 33 29.2-00 49 23 M 13NGC 620516 41 41.4+36 27 37 M 56NGC 677919 16 35.4+30 11 04

Star Star Name --- Element Element --- Z Atomic Number --- Solar Solar abundance (H=12) [] Abundance Abundance of star [] sigma Standard deviation of results [] N number of lines used to derive abundance --- Star Star Name --- Element Element --- Z Atomic Number --- Abundance Abundance of star [] sigma Standard deviation of results [] N Number of lines used to derive abundance --- Element Element --- lambda Wavelength 0.1nm EW(HD165195) HD 165195 equivalent width 0.1pm u_EW(HD165195) Uncertainty flag on EW(HD165195) --- EW(BD+302611) BD +30 2611 equivalent width 0.1pm EW(HD204543) HD 204543 equivalent width 0.1pm EW(HD135148) HD 135148 equivalent width 0.1pm u_EW(HD135148) Uncertainty flag on EW(HD135148) --- Element Element --- Z Atomic Number --- lambda Wavelength 0.1nm loggf Oscillator strength --- r_loggf Reference for loggf number=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) --- EW(BD+112998) BD+11 2998 Equivalent width 0.1pm u_EW(BD+112998) Uncertainty flag on (BD+112998 --- EW(M2V11) M2_V11 equivalent width 0.1pm u_EW(M2V11) Uncertainty flag on (M2V11) --- EW(M2HII89) M2_HII_89 equivalent width 0.1pm u_EW(M2HII89) Uncertainty flag on (M2HII89) --- EW(M13SH11) M13_SH11 equivalent width 0.1pm u_EW(M13SH11) Uncertainty flag on (M13SH11) --- EW(M13I13) M13_I_13 equivalent width 0.1pm u_EW(M13I13) Uncertainty flag on EW(M13I13) --- EW(M56V6) M56_V6 equivalent width 0.1pm u_EW(M56V6) Uncertainty flag on EW(M56V6) --- EW(M56I60) M56_I_60 equivalent width 0.1pm u_EW(M56I60) Uncertainty flag on EW(M56I60) --- EW(M56I96) M56_I_96 equivalent width 0.1pm u_EW(M56I96) Uncertainty flag on EW(M56I96) --- tables.texLaTeX version of the tables Patricia Bauer CDS 1997Jun06Russell, S. C. [Dublin Institute for Advanced Studies] J_A+A_326_1069.xml