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J/ApJ/634/1319  Synthetic Lick indices of alpha-enhanced stars (Franchini+ 2005)

Synthetic Lick indices and detection of α-enhanced stars. III. F, G, and K stars with [Fe/H]>0.00. Franchini M., Morossi C., Di Marcantonio P., Castelli F., Malagnini M.L., Chavez M. <Astrophys. J., 634, 1319-1335 (2005)> =2005ApJ...634.1319F
ADC_Keywords: Abundances ; Stars, late-type Keywords: stellar content - stars: abundances - stars: kinematics - stars: late-type Abstract: A sample of 119 F, G, and K solar neighborhood stars, selected under the condition [Fe/H]>0.00, is investigated in order to detect which of them, if any, present α-enhanced characteristics. According to the kinematics, the sample represents stars of the thin-disk component of the Galaxy. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 75 119 The program stars table4.dat 174 33 *Classification of supersolar stars from the literature
Note on table4.dat: Allende Prieto et al. (2004, Cat. J/A+A/420/183), Fuhrman (2004AN....325....3F), Bensby et al. (2005, Cat. J/A+A/433/185), and Luck & Heiter (2005AJ....129.1063L)
See also: J/ApJS/94/687 : Old stellar populations. V. (Worthey+, 1994) III/232 : STELIB: A library of stellar spectra at R∼2000 (Le Borgne+, 2003) III/218 : ELODIE archive (Prugniel+, 2001) J/AJ/126/2048 : NStars project: the Northern Sample. I. (Gray+, 2003) J/ApJS/152/251 : Indo-US library of coude feed stellar spectra (Valdes+, 2004) J/A+A/420/183 : Spectroscopic survey in solar neighborhood (Allende Prieto+ 2004) J/A+A/433/185 : Detailed abundance analysis of 102 F and G dwarfs (Bensby+, 2005) J/ApJ/613/312 : Synthetic Lick indices of alpha-enhanced stars (Franchini+, 2004) J/ApJ/601/485 : Synthetic Lick indices of alpha-enhanced stars (Franchini+, 2004) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 28 A28 --- Class Classification (1) 30- 35 I6 --- HD HD number 36 A1 --- f_HD [+*] Flag on HD (2) 38- 47 A10 --- SpType MK spectral type 49- 52 F4.2 [Sun] [Fe/H] Average log Fe/H number abundance from the Taylor catalog 54- 57 F4.2 [Sun] e_[Fe/H] Error in [Fe/H] 59 A1 --- LC [gd] Luminosity class: giant (g) or dwarf (d) 61 A1 --- W94 [y-] In the Worthey et al. catalog? (G1) 63 A1 --- C02 [y-] In the Cananea collection data set? (G2) 65 A1 --- STE [y-] In the STELIB library data set? (G3) 67 A1 --- ELO [y-] In the ELODIE library data set? (G4) 69 A1 --- NBP [y-] In the Nearby Stars Project library data set? (G5) 71 A1 --- NSt [y-] In the NStars library data set? (G6) 73 A1 --- I-US [y-] In the Indo-US library data set? (G7) 75 A1 --- S4N [y-] In the Spectroscopic Survey of Stars in the Solar Neighborhood database? (G8)
Note (1): SSA stands for solar scaled abundances, and NSSA for non solar scaled abundances (i.e. α-enhanced stars). Note (2): Flag on HD, defined as follows: + = NSSA classification from Na D vs Ca4227 diagram only. * = SSA classification from Na D vs Mg2 diagram only.
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 6 I6 --- HD The HD number 8- 12 F5.2 [Sun] [Fe/H]T ? [Fe/H] value from Taylor catalog 14- 18 F5.2 [Sun] e_[Fe/H]T ? The RMS error in [Fe/H]_T 20- 24 F5.2 [Sun] dFeT ? Level of supersolar metallicity (1) 26- 30 F5.2 [Sun] [Fe/H]1 ? Allende Prieto et al (2004, Cat. J/A+A/420/183) [Fe/H] value 32- 36 F5.2 [Sun] e_[Fe/H]1 ? The RMS error in [Fe/H]_1 38- 42 F5.2 [Sun] dFe1 ? Difference if >0 (1) 44- 48 F5.2 [Sun] [Fe/H]2 ? Fuhrmann (2004AN....325....3F) [Fe/H] value 50- 54 F5.2 [Sun] e_[Fe/H]2 ? The RMS error in [Fe/H]2 56- 60 F5.2 [Sun] dFe2 ? Difference if >0 (1) 62- 66 F5.2 [Sun] [Fe/H]3 ? Bensby et al. (2005, Cat. J/A+A/433/185) [Fe/H] value 68- 72 F5.2 [Sun] e_[Fe/H]3 ? The RMS error in [Fe/H]3 74- 78 F5.2 [Sun] dFe3 ? Difference if >0 (1) 80- 84 F5.2 [Sun] [Fe/H]4 ? Luck & Heiter (2005AJ....129.1063L) [Fe/H] value 86- 90 F5.2 [Sun] e_[Fe/H]4 ? The RMS error in [Fe/H]4 92- 96 F5.2 [Sun] dFe4 ? Level of supersolar metallicity (1) 98-102 F5.2 [Sun] [Mg/Fe]1 ? Allende Prieto et al (2004, Cat. J/A+A/420/183) [Mg/Fe] value 104-108 F5.2 [Sun] e_[Mg/Fe]1 ? The RMS error in [Mg/Fe]1 110-114 F5.2 [Sun] dMg1 ? Difference if >0 (1) 116-120 F5.2 [Sun] [Mg/Fe]2 ? Fuhrmann (2004AN....325....3F) [Mg/Fe] value 122-126 F5.2 [Sun] e_[Mg/Fe]2 ? The RMS error in [Mg/Fe]2 128-132 F5.2 [Sun] dMg2 ? Difference if >0 (1) 134-138 F5.2 [Sun] [Mg/Fe]3 ? Bensby et al. (2005, Cat. J/A+A/433/185) [Mg/Fe] value 140-144 F5.2 [Sun] e_[Mg/Fe]3 ? The RMS error in [Mg/Fe]3 146-150 F5.2 [Sun] dMg3 ? Difference if >0 (1) 152-156 F5.2 [Sun] [Mg/Fe]4 ? Luck & Heiter (2005AJ....129.1063L) [Mg/Fe] value 158-162 F5.2 [Sun] e_[Mg/Fe]4 ? The RMS error in [Mg/Fe]4 164-168 F5.2 [Sun] dMg4 ? Difference if >0 (1) 170-174 A5 --- Class Star classification (2)
Note (1): Selected stars have abundance determinations satisfying: DiffFe=[Fe/H]-e[Fe/H]>0.0dex, with [Fe/H]>0.0dex DiffMg=[Mg/Fe]-e[Mg/Fe]>0.0dex, with [Mg/Fe]>0.0dex Note (2): Possible classification abbreviated as follows: SSA = high probability solar-scaled abundance SSA: = possible solar-scaled abundance NSSA: = possible non-solar-scaled abundance
Global Notes: Note (G1): Worthey et al. catalog (1994, Cat. J/ApJS/94/687) Note (G2): Cananea collection data set, Moressi et al. (2002ApJ...577..377M) Note (G3): STELIB library (Le Borgne et al., 2003, Cat. III/232) Note (G4): ELODIE library (Prugniel & Soubiran, 2004, Cat. III/218) Note (G5): Nearby Stars Project library (Heiter & Luck 2003AJ....126.2015H; Luck & Heiter 2005AJ....129.1063L) Note (G6): NStars library (Gray et al., 2002, Cat. J/AJ/126/2048) Note (G7): Indo-US library (Valdes et al., 2004, Cat. J/ApJS/152/251) Note (G8): Spectroscopic Survey of Stars in the Solar Neighborhood database (Allende Prieto et al., 2004, Cat. J/A+A/420/183)
History: From electronic version of the journal References: Franchini et al., Paper I 2004ApJ...601..485F, Cat. J/ApJ/601/485 Franchini et al., Paper II 2004ApJ...613..312F, Cat. J/ApJ/613/312
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 08-Aug-2006
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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