/ftp/cats/J_A+A/510/A91/.



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J/A+A/510/A91       V1130 Tau differential uvby light curves    (Clausen+, 2010)
The following files can be converted to FITS (extension .fit or fit.gz)
	table11.dat
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Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/510/A91
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drwxr-xr-x 20 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Dec 15 2013 [TAR file] -rw-r--r-- 1 cats archive 467 May 2 2010 .message -r--r--r-- 1 cats archive 5377 May 2 2010 ReadMe -r--r--r-- 1 cats archive 41976 Dec 17 2009 table11.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/510/A91 V1130 Tau differential uvby light curves (Clausen+, 2010) ================================================================================ Absolute dimensions of eclipsing binaries. XXVII. V1130 Tauri: a metal-weak F-type system, perhaps with preference for Y=0.23-0.24. Clausen J.V., Olsen E.H., Helt B.E., Claret A. <Astron. Astrophys. 510, A91 (2010)> =2010A&A...510A..91C ================================================================================ ADC_Keywords: Binaries, eclipsing ; Photometry, uvby Keywords: stars: evolution - stars: fundamental parameters - stars: individual: V1130 Tau - binaries: eclipsing - techniques: photometric - techniques: radial velocities Abstract: Double-lined, detached eclipsing binaries are our main source for accurate stellar masses and radii. This paper is the first in a series with focus on the upper half of the main-sequence band and tests of 1-2M_sun_ evolutionary models. We aim to determine absolute dimensions and abundances for the detached eclipsing binary V1130 Tau, and to perform a detailed comparison with results from recent stellar evolutionary models. Description: uvby light curves and uvbybeta standard photometry have been obtained with the Stroemgren Automatic Telescope, and high-resolution spectra have been acquired at the FEROS spectrograph; both are ESO, La Silla facilities. We have applied the Wilson-Devinney model for the photometric analysis, spectroscopic elements are based on radial velocities measured via broadening functions, and [Fe/H] abundances have been determined from synthetic spectra and uvby calibrations. Objects: ----------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------- 03 50 41.9 +01 33 50 V1130 Tau = HD 24133 -----------------------------------------------

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