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J/A+A/423/683       Sodium abundances in nearby disk stars   (Shi+, 2004)

Sodium abundances in nearby disk stars. Shi J.R., Gehren T., Zhao G. <Astron. Astrophys., 423, 683-691 (2004)> =2004A&A...423..683S
ADC_Keywords: Stars, nearby ; Abundances, peculiar Keywords: line: formation - line: profiles - stars: abundances - stars: late-type - Galaxy: evolution Abstract: We present sodium abundances for a sample of nearby stars. All results have been derived from NLTE statistical equilibrium calculations. The influence of collisional interactions with electrons and hydrogen atoms is evaluated by comparison of the solar spectrum with very precise fits to the Na I line cores. Description: The spectra of our samples were obtained through the years 1995 to 2000 by Klaus Fuhrmann with the fiber-coupled Cassegrain echelle spectrograph FOCES mounted at the 2.2m telescope of the Calar Alto Observatory. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 42 98 Atmospheric parameters and sodium abundances of the program stars
Table1: Atomic data of Na lines. -------------------------------------------------------------------------------- λ Transition loggf logC6 0.1nm -------------------------------------------------------------------------------- 5682.642 3p 2P01/2 4d 2D3/2 -0.72 -30.05 5688.214 3p 2P03/2 4d 2D5/2 -0.47 -30.05 5889.959 3s 2S1/2 3p 2P01/2 +0.11 -31.60 5895.932 3s 2S1/2 3p 2P03/2 -0.19 -31.60 6154.228 3p 2P01/2 5s 2S1/2 -1.57 -29.78 6160.751 3p 2P03/2 5s 2S1/2 -1.28 -29.78 8183.260 3p 2P01/2 3d 2D3/2 0.28 -30.73 8194.800 3p 2P03/2 3d 2D5/2 0.49 -30.73 -------------------------------------------------------------------------------- Note : loggf values and damping constants have been determined from solar spectrum fits. Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Star name 11- 14 I4 K Teff Effective temperature 16- 19 F4.2 [cm/s2] logg Surface gravity 21- 25 F5.2 Sun [Fe/H] Metallicity 27- 30 F4.2 km/s xi Macroturbulence parameter (1) 32- 36 F5.2 Sun [Na/Fe]LTE LTE value of [Na/Fe] abundance 38- 42 F5.2 Sun [Na/Fe]NLTE NLTE value of [Na/Fe] abundance
Note (1): Rotational velocities and macroturbulence data are the same as in Fuhrmann (1998A&A...338..161F, http://www.xray.mpe.mpg.de/~fuhrmann)
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 26-Aug-2005
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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