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J/A+A/519/A78 BVR light curves of KR Com (Zasche+, 2010)
The following files can be converted to FITS (extension .fit or fit.gz)
bmag.dat rmag.dat vmag.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/519/A78
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drwxr-xr-x 12 cats archive 215 Nov 5 2018 [Up]
drwxr-xr-x 2 cats archive 264 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 480 Dec 19 2022 .message
-r--r--r-- 1 cats archive 2769 Nov 11 2010 ReadMe
-r--r--r-- 1 cats archive 16724 Sep 14 2010 bmag.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 17575 Sep 14 2010 rmag.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 17353 Sep 14 2010 vmag.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/A+A/519/A78 BVR light curves of KR Com (Zasche+, 2010)
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The triple system KR Comae Berenices.
Zasche P., Uhlar R.
<Astron. Astrophys. 519, A78 (2010)>
=2010A&A...519A..78Z
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ADC_Keywords: Binaries, eclipsing ; Photometry, UBVRI ; Photometry, CCD
Keywords: binaries: eclipsing - binaries: visual -
stars: fundamental parameters - stars: individual: KR Com
Abstract:
We present the detailed analysis of triple system KR Com with
different observational techniques - photometry, interferometry, and
period variation.
The use of BVR photometry of the close-contact binary KR Com, which is
the primary component of a triple system, helps us to better describe
the properties of the components. The interferometric data obtained
during the last 30 years sufficiently determine the visual orbit, but
the use of minima timings of KR Com for the study of period variation
together with the visual orbit is a novel approach in this system.
Description:
Original CCD photometry in B, V, and R filters for the eclipsing
binary system KR Com.
Objects:
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RA (2000) DE Designation(s)
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13 20 15.8 +17 45 57 KR Com = HD 115955
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