Show | Sort | Column | Constraint | Explain (UCD) |
| | recno | | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) (RECORD) |
| | ID | (char) | Identifier name from NGC 6752 IDs and 2MASS JHHMMSS.ss+DDMMSS.s designation (IDs) (meta.id;meta.main) (ID_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) (PHYS_TEMP_EFFEC) |
| | e_Teff | K | Derived uncertainty of Teff as explained in the section 3.5 Observational uncertainties (s_Teff) (stat.error;phys.temperature.effective) (ERROR) |
| | 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) (PHYS_GRAVITY_SURFACE) |
| | e_logg | [cm/s2] | Derived uncertainty of logg as explained in the section 3.5 Observational uncertainties (s_logg) (stat.error) (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) (PHYS_ABUND_FE/H) |
| | 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) (ERROR) |
| | 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) (VELOC_MICRO-TURB) |
| | e_vt | km/s | Derived uncertainty of vt as explained in the section 3.5 Observational uncertainties (s_vm) (stat.error) (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) (PHYS_ABUND_MISC) |
| | e_A(Li) | [-] | Derived uncertainty of A(Li) as explained in the section 3.5 Observational uncertainties (s_Li) (stat.error) (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) (PHYS_ABUND_MISC) |
| | e_[Al/Fe] | [-] | Derived uncertainty of [Al/Fe] as explained in the section 3.5 Observational uncertainties (s_Al) (stat.error;phys.abund) (ERROR) |
| | 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) (DATA_LINK) |
| | _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) (POS_EQ_RA_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) (POS_EQ_DEC_MAIN) |
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