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 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:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table5.dat 50 152 Fundamental parameters of observed stars
table6.dat 182 152 Determined abundances of observed stars
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Byte-by-byte Description of file: table5.dat
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Bytes Format Units Label Explanations
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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)
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Byte-by-byte Description of file: table6.dat
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Bytes Format Units Label Explanations
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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)
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Global notes:
Note (G1): Name of the spectrograph used is
c = CORALIE;
e = ELODIE
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Acknowledgements:
Pierre North
References:
Erspamer and North, Paper I 2002A&A...383..227E 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