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J/A+A/502/253         V636 Cen radial velocities curves         (Clausen+, 2009)

Absolute dimensions of solar-type eclipsing binaries. II. V636 Centauri: A 1.05M primary with an active, cool, oversize 0.85M secondary. Clausen J.V., Bruntt H., Claret A., Larsen A., Andersen J., Nordstrom B., Gimenez A. <Astron. Astrophys. 502, 253 (2009)> =2009A&A...502..253C
ADC_Keywords: Binaries, eclipsing ; Radial velocities Keywords: stars: evolution - stars: fundamental parameters - stars: abundances - stars: activity - stars: binaries: eclipsing - techniques: spectroscopic Abstract: The influence of stellar activity on the fundamental properties of stars around and below 1M is not well understood. Accurate mass, radius, and abundance determinations from solar-type binaries exhibiting various levels of activity are needed for a better insight into the structure and evolution of these stars. We aim to determine absolute dimensions and abundances for the solar-type detached eclipsing binary V636Cen, and to perform a detailed comparison with results from recent stellar evolutionary models. uvby light curves and uvbyβ standard photometry were obtained with the Stroemgren Automatic Telescope, radial velocity observations with the CORAVEL spectrometer, and high-resolution spectra with the FEROS spectrograph, all at ESO, La Silla. State-of-the-art methods were applied for the photometric and spectroscopic analyses. Description: Radial velocities of V636 Cen and residuals from the final spectroscopic orbit. Objects: ------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------ 14 16 57.9 -49 56 42 V636 Cen = HD 124784 ------------------------------------------------ File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tablea1.dat 74 39 Radial velocities of V636 Cen and residuals from the final spectroscopic orbit
See also: J/A+A/487/1081 : uvby photometry of 6 eclipsing binaries (Clausen+, 2008) Byte-by-byte Description of file: tablea1.dat
Bytes Format Units Label Explanations
1- 11 F11.3 d HJD(p) ? Heliocentric Julian Date primary component 13- 18 F6.4 --- Phase(p) ? Orbital phase, primary component 20- 25 F6.2 km/s RV(p) ? Radial velocity, primary component 27- 30 F4.2 km/s e_RV(p) ? Internal velocity error, primary component 32- 36 F5.2 km/s O-C(p) ? Observed-calculated velocity residual, primary component 38- 48 F11.3 d HJD(s) Heliocentric Julian Date secondary component 50- 55 F6.4 --- Phase(s) Orbital phase, secondary component 57- 63 F7.2 km/s RV(s) Radial velocity, secondary component 65- 68 F4.2 km/s e_RV(s) Internal velocity error, secondary component 70- 74 F5.2 km/s O-C(s) Observed-calculated velocity residual, secondary component
Acknowledgements: jvc(at)astro.ku.dk References: Clausen et al., Paper I 2001A&A...374..980C
(End) J.V. Clausen [Niels Bohr Inst., Copenhagen], P. Vannier [CDS] 22-May-2009
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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