VizieR

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VizieR

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J/MNRAS/511/231
  Lithium study with GC NGC 6752 (Schiappacasse-Ulloa+, 2022)
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2022MNRAS.511..231S
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1.J/MNRAS/511/231/table1Stellar parameters of our stars sample in the metal-poor globular cluster NGC 6752 (217 rows)

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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  ID (char) Identifier name from NGC 6752 IDs and 2MASS JHHMMSS.ss+DDMMSS.s designation (IDs) (meta.id;meta.main)
  Teff K Effective temperature derived as explicited in sections 3.1 Photometric stellar parameters and 3.2 Spectroscopic stellar parameters (Teff) (phys.temperature.effective)
  e_Teff K Derived uncertainty of Teff as explained in the section 3.5 Observational uncertainties (s_Teff) (stat.error;phys.temperature.effective)
  logg [cm/s2] Logarithm of the surface gravity derived as explicited in sections 3.1 Photometric stellar parameters and 3.2 Spectroscopic stellar parameters (logg) (phys.gravity)
  e_logg [cm/s2] Derived uncertainty of logg as explained in the section 3.5 Observational uncertainties (s_logg) (stat.error)
  [Fe/H] [Sun] Iron to hydrogen abundance ratio adopted value -1.56 as explicited in sections 3.1 Photometric stellar parameters and 3.2 Spectroscopic stellar parameters (Fe_H) (phys.abund.Fe;arith.ratio)
  e_[Fe/H] [Sun] Derived uncertainty 0.01 dex of [Fe/H] as explained in the section 3.5 Observational uncertainties (s_Fe) (stat.error;phys.abund.Fe)
  vt km/s Microturbulence velocity derived as explicited in sections 3.1 Photometric stellar parameters and 3.2 Spectroscopic stellar parameters (vm_2) (phys.veloc.microTurb)
  e_vt km/s Derived uncertainty of vt as explained in the section 3.5 Observational uncertainties (s_vm) (stat.error)
  A(Li) [-] Lithium abundances as A(Li) = log(NLi/NH)+12 derived with equivalent widths measurements from spectroscopic analysis as explained in the section 3.2 Spectroscopic stellar parameters and 3.4 Measurement of Li and Al (Li1) (phys.abund)
  e_A(Li) [-] Derived uncertainty of A(Li) as explained in the section 3.5 Observational uncertainties (s_Li) (stat.error)
  [Al/Fe] [-] Aluminium to iron abundance ratio derived with equivalent widths measurements from spectroscopic analysis as explained in the section 3.2 Spectroscopic stellar parameters and 3.4 Measurement of Li and Al (Al_Fe1) (phys.abund)
  e_[Al/Fe] [-] Derived uncertainty of [Al/Fe] as explained in the section 3.5 Observational uncertainties (s_Al) (stat.error;phys.abund)
  Link  Link to see the catalog of stellar parameters and abundances in NGC 6752 by Gruyters et al. 2014A&A...567A..72G, Cat. J/A+A/567/A72 (meta.ref.url)
  _RA deg (i) Position from Gruyters et al. 2014A&A...567A..72G, Cat. J/A+A/567/A72 and from names 2MASS JHHMMSS.ss+DDMMSS.s (right ascension part) (pos.eq.ra;meta.main)
  _DE deg (i) Position from Gruyters et al. 2014A&A...567A..72G, Cat. J/A+A/567/A72 and from names 2MASS JHHMMSS.ss+DDMMSS.s (declination part) (pos.eq.dec;meta.main)

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