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Table C.3
Stellar parameters, ages, abundance ratios, uncertainties, and kinematical properties for the 714 stars.
Column | Label | Unit | Comment |
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(1) | HIP | ||
(2) | Spec | Spectrograph | |
(3) | Teff | K | |
(4) | ϵ(Teff) | K | |
(5) | log g | ||
(6) | ϵ(log g) | ||
(7) | ξt | km s-1 | |
(8) | ϵ(ξt) | km s-1 | |
(9) | log ε(Fe i) | Absolute abundance from Fe i lines | |
(10) | log ε(Fe ii) | Absolute abundance from Fe ii lines | |
(11) | mass | sun | Best mass |
(12) | massl | sun | Lower limit on mass |
(13) | massu | sun | Upper limit on mass |
(14) | Age | Gyr | Best age |
(15) | Agel | Gyr | Lower limit on age |
(16) | Ageu | Gyr | Upper limit on age |
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(17) | [Fe/H] | Sun | |
(18) | [O/Fe] | Sun | |
(19) | [Na/Fe] | Sun | |
(20) | [Mg/Fe] | Sun | |
(21) | [Al/Fe] | Sun | |
(22) | [Si/Fe] | Sun | |
(23) | [Ca/Fe] | Sun | |
(24) | [Ti/Fe] | Sun | |
(25) | [Cr/Fe] | Sun | |
(26) | [Ni/Fe] | Sun | |
(27) | [Zn/Fe] | Sun | |
(28) | [Y/Fe] | Sun | |
(29) | [Ba/Fe] | Sun | |
(30) | ϵ [Fe/H] | Abundance ratio uncertainty | |
(31) | ϵ [O/Fe] | ||
(32) | ϵ [Na/Fe] | ||
(33) | ϵ [Mg/Fe] | ||
(34) | ϵ [Al/Fe] | ||
(35) | ϵ [Si/Fe] | ||
(36) | ϵ [Ca/Fe] | ||
(37) | ϵ [Ti/Fe] | ||
(38) | ϵ [Cr/Fe] | ||
(39) | ϵ [Ni/Fe] | ||
(40) | ϵ [Zn/Fe] | ||
(41) | ϵ [Y/Fe] | ||
(42) | ϵ [Ba/Fe] | ||
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(43) | [Ti/H] | Sun | |
(44) | [O/Ti] | Sun | |
(45) | [Na/Ti] | Sun | |
(46) | [Mg/Ti] | Sun | |
(47) | [Al/Ti] | Sun | |
(48) | [Si/Ti] | Sun | |
(49) | [Ca/Ti] | Sun | |
(50) | [Cr/Ti] | Sun | |
(51) | [Ni/Ti] | Sun | |
(52) | [Fe/Ti] | Sun | |
(53) | [Zn/Ti] | Sun | |
(54) | [Y/Ti] | Sun | |
(55) | [Ba/Ti] | Sun | |
(56) | ϵ [Ti/H] | Abundance ratio uncertainty | |
(57) | ϵ [O/Ti] | ||
(58) | ϵ [Na/Ti] | ||
(59) | ϵ [Mg/Ti] | ||
(60) | ϵ [Al/Ti] | ||
(61) | ϵ [Si/Ti] | ||
(62) | ϵ [Ca/Ti] | ||
(63) | ϵ [Cr/Ti] | ||
(64) | ϵ [Ni/Ti] | ||
(65) | ϵ [Fe/Ti] | ||
(66) | ϵ [Zn/Ti] | ||
(67) | ϵ [Y/Ti] | ||
(68) | ϵ [Ba/Ti] | ||
(69) | N(Fe i) | Number of lines used | |
(70) | N(Fe ii) | ||
(71) | N(O i) | ||
(72) | N(Na i) | ||
(73) | N(Mg i) | ||
(74) | N(Al i) | ||
(75) | N(Si i) | ||
(76) | N(Ca i) | ||
(77) | N(Ti i) | ||
(78) | N(Ti ii) | ||
(79) | N(Cr i) | ||
(80) | N(Cr ii) | ||
(81) | N(Ni i) | ||
(82) | N(Zn i) | ||
(83) | N(Y ii) | ||
(84) | N(Ba ii) | ||
(85) | σ(Fe i) | 1-σ line-to-line dispersion | |
(86) | σ(Fe ii) | ||
(87) | σ(O i) | ||
(88) | σ(Na i) | ||
(89) | σ(Mg i) | ||
(90) | σ(Mg i) | ||
(91) | σ(Si i) | ||
(92) | σ(Ca i) | ||
(93) | σ(Ti i) | ||
(94) | σ(Ti ii) | ||
(95) | σ(Cr i) | ||
(96) | σ(Cr ii) | ||
(97) | σ(Ni i) | ||
(98) | σ(Zn i) | ||
(99) | σ(Y ii) | ||
(100) | σ(Ba ii) | ||
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(101) | π | mas | Hipparcos plx |
(102) | σπ | mas | plx uncertainty |
(103) | d | kpc | Distance |
(104) | l | deg | Galactic longitude |
(105) | b | deg | Galactic latitude |
(106) | ULSR | km s-1 | |
(107) | VLSR | km s-1 | |
(108) | WLSR | km s-1 | |
(109) | Rmin | kpc | |
(110) | Rmax | kpc | |
(111) | zmax | kpc | |
(112) | e | ||
(113) | LZ | ||
(114) | E/ELSR | Total energy normalised to the LSR | |
(115) | TD/D | ||
(116) | TD/H | ||
(117) | Her/TD | ||
(118) | Her/D | ||
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(119) | Teff (u.i.b) | K | Un-corrected ion.bal temp |
(120) | log g (u.i.b) | Un-corrected ion.bal grav | |
(121) | Teff (hip) | K | Hipparcos temp |
(122) | log g (hip) | Hipparcos grav | |
(123) | log ε(Fe i) (hip) | Absolute abundance using Hipparcos plx | |
(124) | log ε(Fe ii) (hip) | Absolute abundance using Hipparcos plx |
Notes. The table is only available in electronic form at the CDS.
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