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J/A+A/398/1121      Abundances of A-F stars                 (Erspamer+, 2003)

Automated Spectroscopic abundances of A and F-type stars using echelle spectrographs. II. Abundances of 140 A-F stars from ELODIE and CORALIE. Erspamer D., North P. <Astron. Astrophys. 398, 1121 (2003)> =2003A&A...398.1121E
ADC_Keywords: Stars, A-type ; Stars, F-type ; Abundances, peculiar Keywords: techniques: spectroscopic - stars: abundances - stars: chemically peculiar - stars: fundamental parameters Description: Fundamental parameters and abundances of 140 A and F-type stars are presented. The barycentric Julian dates and signal-to-noise ratios are also given. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table5.dat 50 152 Fundamental parameters of observed stars table6.dat 182 152 Determined abundances of observed stars
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 6 I6 --- HD HD (Cat. III/135) number 8- 12 I5 K Teff Effective Temperature 14- 17 F4.2 [cm/s2] log(g) Logarithm of the surface gravity 19- 29 F11.3 d BJD Barycentric Julian day 31- 36 F6.2 km/s RV Radial velocity 38- 40 I3 km/s Vsini Projected rotational velocity 42- 44 F3.1 km/s xi Microturbulent velocity 46- 48 I3 --- S/N Signal-to-noise ratio at 5550Å 50 A1 --- S1 [ce] Name of the spectrograph used (G1)
Byte-by-byte Description of file: table6.dat
Bytes Format Units Label Explanations
1- 6 I6 --- HD HD number 8- 12 F5.2 [Sun] He ? He (Z=2) abundance 14- 18 F5.2 [Sun] C C (Z=6) abundance 20- 24 F5.2 [Sun] O ? O (Z=6) abundance 26- 30 F5.2 [Sun] Na ? Na (Z=11) abundance 32- 36 F5.2 [Sun] Mg Mg (Z=12) abundance 38- 42 F5.2 [Sun] Al ? Al (Z=13) abundance 44- 48 F5.2 [Sun] Si Si (Z=14) abundance 50- 54 F5.2 [Sun] S ? S (Z=16) abundance 56- 60 F5.2 [Sun] Ca Ca (Z=20) abundance 62- 66 F5.2 [Sun] Sc Sc (Z=21) abundance 68- 72 F5.2 [Sun] Ti Ti (Z=22) abundance 74- 78 F5.2 [Sun] V ? V (Z=23) abundance 80- 84 F5.2 [Sun] Cr Cr (Z=24) abundance 86- 90 F5.2 [Sun] Mn ? Mn (Z=25) abundance 92- 96 F5.2 [Sun] Fe Fe (Z=26) abundance 98-102 F5.2 [Sun] Co ? Co (Z=27) abundance 104-108 F5.2 [Sun] Ni ? Ni (Z=28) abundance 110-114 F5.2 [Sun] Cu ? Cu (Z=29) abundance 116-120 F5.2 [Sun] Zn ? Zn (Z=30) abundance 122-126 F5.2 [Sun] Sr ? Sr (Z=38) abundance 128-132 F5.2 [Sun] Y ? Y (Z=39) abundance 134-138 F5.2 [Sun] Zr ? Zr (Z=40) abundance 140-144 F5.2 [Sun] Ba ? Ba (Z=56) abundance 146-150 F5.2 [Sun] La ? La (Z=57) abundance 152-156 F5.2 [Sun] Ce ? Ce (Z=58) abundance 158-162 F5.2 [Sun] Pr ? Pr (Z=59) abundance 164-168 F5.2 [Sun] Nd ? Nd (Z=60) abundance 170-174 F5.2 [Sun] Sm ? Sm (Z=62) abundance 176-180 F5.2 [Sun] Eu ? Eu (Z=63) abundance 182 A1 --- S2 [ce] Name of the spectrograph used (G1)
Global notes: Note (G1): Name of the spectrograph used is c = CORALIE; e = ELODIE
Acknowledgements: Pierre North References: Erspamer and North, Paper I 2002A&A...383..227E History: * 31-Jan-2003: Original version * 12-Oct-2009: table5 corrected (from author): concerns the effective temperatures of the 2 stars HD 15318 and 108767.
(End) Patricia Bauer [CDS] 07-Oct-2002
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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