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J/A+A/282/831     Spectroscopic orbits of three K dwarf stars  (Tokovinin+ 1994)

Duplicity in the solar neighbourhood. VII. Spectroscopic orbits of three K-dwarfs stars Tokovinin A.A., Duquennoy A., Halbwachs J.-L., Mayor M. <Astron. Astrophys. 282, 831 (1994)> =1994A&A...282..831T
ADC_Keywords: Binaries, spectroscopic; Radial velocities; Stars, K-type Keywords: techniques: radial velocities - binaries: spectroscopic - stars: late type - stars individual : HD 23439B, HD 237287, HD 217580 Description: The spectroscopic orbits of single-lined binary dwarfs HD 23439B, HD 237287 and HD 217580 are derived from the radial velocities measured with two correlation radial-velocity spectrometers: correlation radial velocity (CORAVEL) at the 1m Swiss telescope of Observatoire de Haute-Provence, and radial velocity meters (RVM) used on several telescopes. The mutual agreement of these two data sets is analyzed and found to be quite good. The estimated minimum mass of secondary component corresponds to that of M-type dwarf for the first 2 systems and is equal to 0.06 solar mass for HD 217580. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 03 47 02.7 +41 25 42 HD 23439B = Gliese 1064B 04 36 06.2 +55 24 44 HD 237287 = Gliese 171 23 01 51.5 -03 50 55 HD 217580 = Gliese 886 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 38 43 Observations and residuals of HD 23439B table5.dat 38 38 Observations and residuals of HD 237287 table6.dat 37 62 Observations and residuals of HD 217580
Byte-by-byte Description of file: table4.dat table5.dat table6.dat
Bytes Format Units Label Explanations
1- 11 F11.3 d HJD Heliocentric Julian Date 13- 18 F6.2 km/s Vr Radial velocity 24- 27 F4.2 km/s e_Vr Uncertaincy on radial velocity 29- 33 F5.2 km/s O-C Velocity residual (Observed-Computed) 35- 37 A3 --- Inst Instrument CORAVEL (COR) or RVM (1)
Note (1): the RVM velocities have been increased by 0.4 km/s

(End) Patricia Bauer [CDS] 01-Mar-1994
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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