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J/A+A/376/158 SV Cam BVR light curves (Albayrak+, 2001)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
table1.dat
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Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=J/A+A/376/158
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drwxr-xr-x 18 cats archive 323 Jan 29 2012 [Up]
drwxr-xr-x 2 cats archive 293 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 469 Dec 19 2022 .message
-r--r--r-- 1 cats archive 2931 Sep 9 2001 ReadMe
-rw-r--r-- 1 cats archive 213 Sep 19 2007 +footg5.gif
-rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif
-r--r--r-- 1 cats archive 2416 Jul 13 2001 table1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 8463 Jul 13 2001 table1.ps.gz [Uncompressed]
-r--r--r-- 1 cats archive 2995 Jul 13 2001 table1.tex.gz [Uncompressed]
Beginning of ReadMe :J/A+A/376/158 SV Cam BVR light curves (Albayrak+, 2001)
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A light and period study of SV Camelopardalis
Albayrak B., Demircan O., Djurasevic G., Erkapic S., Ak H.
<Astron. Astrophys. 376, 158 (2001)>
=2001A&A...376..158A
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ADC_Keywords: Binaries, eclipsing ; Photometry
Keywords: stars: binaries: eclipsing - stars: individual: SV Cam
Abstract:
New BVR light curves and times of minimum light for the short period
RS CVn system SV Cam were analysed to derive the physical parameters
of the system and the parameters of the third body orbit. The light
curves obtained at the TUEBITAK National Observatory during two nights
in 2000 show considerable asymmetry and night-to-night variations. The
analysis of the light curves is made using Djurasevic's inverse
problem method. The Roche model with spotted areas on the hotter
primary component yields a good fit to observations. The extensive
series of published photoelectric minima times indicate that the
eclipsing pair orbits around the common mass center of the triple
system with a period of 41.32yr.
Objects:
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RA (2000) DE Designation(s)
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06 41 19.1 +82 16 02 SV Cam
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