J/A+A/464/927       Abundances of red giants in NGC 6752       (Carretta+, 2007)
Na-O Anticorrelation and HB.
II. The Na-O anticorrelation in the globular cluster NGC 6752
    Carretta E., Bragaglia A., Gratton R.G., Lucatello S., Momany Y.
   <Astron. Astrophys. 464, 927 (2007)>
   =2007A&A...464..927C 2007A&A...464..927C
ADC_Keywords: Clusters, globular ; Stars, population II ; Abundances ;
              Radial velocities
Keywords: stars: abundances - stars: atmospheres - stars: Population II -
          Galaxy: globular clusters: general -
          Galaxy: globular clusters: individual: NGC 6752
Abstract:
    We are studying the Na-O anticorrelation in several globular clusters
    of different Horizontal Branch (HB) morphology in order to derive a
    possible relation between (primordial) chemical inhomogeneities and
    morphological parameters of the cluster population.
    We used the multifiber spectrograph FLAMES on the ESO Very Large
    Telescope UT2 and derived atmospheric parameters and elemental
    abundances of Fe, O and Na for about 150 red giant stars in the
    Galactic globular cluster NGC 6752.
    The average metallicity we derive is [Fe/H]=-1.56, in agreement with
    other results from red giants, but lower than obtained for dwarfs or
    early subgiants.
    In NGC 6752 there is not much space for an intrinsic spread in
    metallicity: on average, the rms scatter in [Fe/H] is
    0.037±0.003dex, while the scatter expected on the basis of the major
    error sources is 0.039±0.003dex.
    The distribution of stars along the Na-O anticorrelation is different
    to what was found in the first paper of this series for the globular
    cluster NGC 2808: in NGC 6752 it is skewed toward more Na-poor stars,
    and it resembles more the one in M 13.
    Detailed modeling is required to clarify whether this difference may
    explain the very different distributions of stars along the HB.
Description:
    Spectra for 151 RGB stars in NGC 6752 were obtained with FLAMES@VLT
    using two gratings (HR11, HR13). Abundances of Fe, O, Na were derived
    using equivalent widths, model atmospheres and atmospheric parameters
    based on photometry.
    For each star we give identification, equatorial coordinates, VBJK
    magnitudes, S/N, heliocentric radial velocity for both gratings, Teff,
    logg, [A/H], vt, [Fe/H], [O/Fe], [Na/Fe]. Equivalent widths are
    given in tablea.
File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
table2.dat     88      151   Identification, equatorial coordinates, VBJK
                              magnitudes, S/N, heliocentric radial velocity
table3.dat     54      137   Atmospheric parameters and iron abundance
table5.dat     37      137   O and Na abundances
tablea.dat     37     8220   Equivalent widths for 137 objects
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See also:
    J/A+A/455/271 : Abundances of red giants in NGC 6441 (Gratton+, 2006)
    J/A+A/464/939 : Abundances of red giants in NGC 6218 (Carreta+, 2007)
    J/A+A/464/953 : Abundances of red giants in NGC 6441 (Gratton+, 2007)
    J/A+A/464/967 : Abundances of red giants in NGC 6388 (Carreta+, 2007)
Byte-by-byte Description of file: table2.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label    Explanations
--------------------------------------------------------------------------------
   2-  6  I5    ---     ID       Identification (from Momany et al.,
                                  2004A&A...420..605M 2004A&A...420..605M)
   8-  9  I2    h       RAh      Right ascension (J2000.0)
  11- 12  I2    min     RAm      Right ascension (J2000.0)
  14- 19  F6.3  s       RAs      Right ascension (J2000.0)
      21  A1    ---     DE-      Declination sign (J2000.0)
  22- 23  I2    deg     DEd      Declination (J2000.0)
  25- 26  I2    arcmin  DEm      Declination (J2000.0)
  28- 32  F5.2  arcsec  DEs      Declination (J2000.0)
  34- 39  F6.3  mag     Vmag     ? Johnson V magnitude
  41- 46  F6.3  mag     Bmag     ? Johnson B magnitude
  48- 53  F6.3  mag     Jmag     ? 2MASS J magnitude
  55- 60  F6.3  mag     Kmag     ? 2MASS J magnitude
  62- 64  I3    ---     S/N      Signal-to-Noise ratio
  66- 71  F6.2  km/s    HRV11    ? Heliocentric radial velocity for grating HR11
  73- 78  F6.2  km/s    HRV13    ? Heliocentric radial velocity for grating HR13
  80- 84  A5    ---     HR       [11,13 ] Grating(s) used
  86- 88  A3    ---     Flag     [F*+, ] Notes (1)
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Note (1): Notes as follows:
      F = field star
      * = stars with unreliable V-K
      + = not used in analysis
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Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   2-  6  I5    ---     ID        Identification (from Momany et al.,
                                   2004A&A...420..605M 2004A&A...420..605M)
   8- 11  I4    K       Teff      Effective temperature
  13- 16  F4.2  [cm/s2] logg      Gravity
  18- 22  F5.2  [Sun]   [A/H]     Metallicity
  24- 27  F4.2  km/s    Vt        Microturbulent velocity
  29- 30  I2    --    o_FeI       Number of lines of Fe I
  32- 36  F5.2  [Sun]   [Fe/H]I   Average star [Fe/H]I
  38- 41  F4.2  [Sun] e_[Fe/H]I   rms uncertainty on [Fe/H]I
      43  I1    --    o_FeII      ? Number of lines of Fe II
  45- 49  F5.2  [Sun]   [Fe/H]II  ? Average star [Fe/H]II
  51- 54  F4.2  [Sun] e_[Fe/H]II  ? rms uncertainty on [Fe/H]II
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Byte-by-byte Description of file: table5.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   2-  6  I5    ---     ID        Identification (from Momany et al.,
                                   2004A&A...420..605M 2004A&A...420..605M)
       8  I1    ---   o_O         ? Number of lines of O
  10- 14  F5.2  [Sun]   [O/Fe]    ? Average [O/Fe]
  16- 19  F4.2  [Sun] e_[O/Fe]    ? rms uncertainty on [O/Fe]
      22  I1    ---   o_Na        ? Number of lines of Na
  24- 28  F5.2  [Sun]   [Na/Fe]   ? Average [Na/Fe]
  30- 33  F4.2  [Sun] e_[Na/Fe]   ? rms uncertainty on [Na/Fe]
      35  I1    ---     Flag1     [1/3] Flag for grating (1)
      37  I1    --      Flag2     [0/1] Flag for measure/limit for O (2)
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Note (1): Flags for grating as follows:
      1 = HR13 only
      2 = both HR11 & HR13
      3 = only HR11
Note (2): Flags for measure/limit for O as follows:
      0 = O upper limit
      1 = O measured
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Byte-by-byte Description of file: tablea.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  5  I5    ----    ID        Identification (from Momany et al.,
                                   2004A&A...420..605M 2004A&A...420..605M)
   7- 10  F4.1  ---     ---       Atomic number and ionization stage (1)
  13- 19  F7.2  0.1nm   lambda    Wavelength
  21- 24  F4.2  eV      EP        Excitation potential
  26- 31  F6.2  [cm/s2] loggf     Surface gravity
  33- 37  F5.1  0.1pm   EW        Equivalent width
--------------------------------------------------------------------------------
Note (1): NN.1 for neutral, NN.2 for singly ionized
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Acknowledgements:
    Eugenio Carretta, eugenio.carretta(at)oabo.inaf.it
References:
  Carreta et al., Paper I,   NGC 2808  2006A&A...450..523C 2006A&A...450..523C
  Gratton et al., Paper III, NGC 6441  2006A&A...455..271G 2006A&A...455..271G, Cat. J/A+A/455/271
  Carreta et al., Paper IV,  NGC 6218  2007A&A...464..939C 2007A&A...464..939C, Cat. J/A+A/464/939
  Gratton et al., Paper V,   NGC 6441  2007A&A...464..953G 2007A&A...464..953G, Cat. J/A+A/464/953
  Carreta et al., Paper VI,  NGC 6388  2007A&A...464..967C 2007A&A...464..967C, Cat. J/A+A/464/967
(End)                                        Patricia Vannier [CDS]  22-Feb-2007