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J/other/NewA/17.296       GO Cyg BV light curves                (Ulas+, 2012)

Close binary system GO Cyg. Ulas B., Kalomeni B., Keskin V., Kose O., Yakut K. <New Astron. 17 296 (2012)> =2012NewA...17..296U
ADC_Keywords: Binaries, eclipsing ; Photometry, UBV Keywords: stars: binaries: eclipsing - stars: binaries: close - stars: binaries: general - stars: fundamental parameters - stars: low-mass Abstract: In this study, we present long term photometric variations of the close binary system GO Cyg. Modelling of the system shows that the primary is filling Roche lobe and the secondary of the system is almost filling its Roche lobe. The physical parameters of the system are M1=3.0±0.2M, M2=1.3±0.1M, R1=2.50±0.12R, R2=1.75±0.09R, L1=64±9L, L2=4.9±0.7L, and a=5.5±0.3R. Our results show that GO Cyg is the most massive system near contact binary (NCB). Analysis of times of the minima shows a sinusoidal variation with a period of 92.3±0.5-years due to a third body whose mass is less than 2.3M. Finally a period variation rate of -1.4x10-9d/yr has been determined using all available light curves. Description: Photometric variations of the close binary system GO Cyg is presented. Physical and orbital parameters of the system are determined. It is found that the the system is the most massive among near contact binaries. Objects: -------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------- 20 37 20.1 +35 26 10 GO Cyg = V* GO Cyg -------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 101 16 Available light curves of GO Cyg that are collected from the literature table5.dat 34 5417 Available light curves data
See also: J/other/NewA/17.46 : VRI light curves of V1191 Cyg (Ulas+, 2012) Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 4 A4 --- LC Light curve designation (1) 6- 12 A7 --- Date Date of observation (Year) 14- 20 F7.1 d JD1 ? Time interval (JD-2400000) 21 A1 --- --- [-] 22- 28 F7.1 d JD2 ? Time interval (JD-2400000) 30- 38 A9 --- Filt Filters used 40- 42 A3 --- Type Type of observation (pg, pe, ccd) 44- 77 A34 --- Comp Comparison star(s) 79- 99 A21 --- Npts Number of data points be filters 101 A1 --- Data [Y/N] Data availability
Note (1): References for the light curves: LC01 = Payne-Gaposchkin (1935, BHarO 898, 3) LC02 = Liau (1935, POLyo, 1) LC03 = Pierce (1939, AJ 48, 113) LC04 = Popper (1957ApJS....3..107P) LC05 = Ovenden (1954MNRAS.114..569O) LC06 = Mannino (1963MmSAI..34..191M) LC07 = Sezer et al. (1993Ap&SS.203..121S) LC08 = Rovithis et al. (1990A&AS...83...41R) LC09 = Oprescu et al. (1996RoAJ....6..119O) LC10 = Jassur (1997Ap&SS.249..111J) LC11 = Rovithis-Livaniou et al. (1997A&A...327.1017R) LC12 = Edalati and Atighi (1997Ap&SS.253..107E) LC13 = Vukasovic (1997, IAPPP 67, 11) LC14 = Oh et al. (2000Ap&SS.271..303K) LC15 = Zabihinpoor et al. (2010PASP..122..309Z) LC16 = This study
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 4 A4 --- LC Light curve designation 6 A1 --- Filt [BV] Filter 8- 19 F12.4 d JD ? Julian date (1) 21- 27 F7.4 --- Phase ? Orbital phase (1) 29- 34 F6.3 mag Dmag Differential magnitude (2)
Note (1): Phases are given for the light curves LC3, LC5, and LC15 since JDs are not provided. P0=0.717764585(15)d. Note (2): Magnitude differences between variable and comparison stars. Comparison stars are listed in Table 3.
Acknowledgements: Burak Ulas, bulash(at)gmail.com
(End) Burak Ulas [EU], Patricia Vannier [CDS] 02-Dec-2011
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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