J/MNRAS/253/610 Li abundances for 81 F dwarfs (Lambert+, 1991)
Lithium abundances for 81 F dwarfs.
Lambert D.L., Heath J.E., Edvardsson B.
<Mon. Not. R. Astron. Soc., 253, 610-610 (1991)>
=1991MNRAS.253..610L 1991MNRAS.253..610L
ADC_Keywords: Stars, dwarfs ; Abundances
Abstract:
Lithium abundances are presented for 81 main-sequence stars with
effective temperatures of about 5800-6700K.
Description:
All observations where made at the W.J. McDonald Observatory with the
coude spectrographs of the 2.1m and 2.7m reflectors.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 61 81 Equivalent width of lithium lines
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See also:
J/A+AS/102/603 : Chemical evolution of the galactic disk II. (Edvardsson+ 1993)
Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 9 A9 --- Name Star name
12- 13 I2 0.1pm EW6703 Equivalent width at 6703Å (mÅ)
16- 17 I2 0.1pm EW6705 Equivalent width at 6705Å (mÅ)
19 A1 --- l_EW6707 Limit flag on EW6707
20- 24 F5.1 0.1pm EW6707 Equivalent width at 6707Å (mÅ)
26- 29 I4 K Teff Effective temperature
32- 35 F4.2 [cm/s2] logg Surface gravity
38- 41 F4.2 mag VMAG Absolute V magnitude
44- 47 F4.2 solMass Mass ?=- Mass (1)
50- 54 F5.2 [Sun] [Fe/H] Metallicity
55 A1 --- n_[Fe/H] [b] [Fe/H] computed from photometry (2)
57 A1 --- l_loge(Li) Limit flag on loge(Li)
58- 61 F4.2 --- loge(Li) Lithium abundance (scale H=12)
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Note (1): Estimated masses for stars with VMAG≥3.60.
Note (2): b = [Fe/H] is computed from Stroemgren photometry.
All other entries are spectroscopic estimates from
Edvardsson et al. (1993, Cat. J/A+AS/102/603)
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Acknowledgements:
Eric E. Mamajek, emamajek(at)pas.rochester.edu
(End) Patricia Vannier [CDS] 12-Jan-2009