From photoelectric and spectroscopic data available in the literature, we bave determined the elements of three. W Ursae Majoris systems, by means of the Roche-model-based method of Wilson and Devinney. According to our solutions, the three systems (V757 Cen, ER Cep, AH Cnc) are a11 of W-type, that is primary minima are caused by occultation of the smaller (and less massive) component
Spectroscopic elements of the W UMa system HD 101799 were derived from radial velocity observations....
The UBV photometry of the short period binary FM Vel is analysed by means of the method of Wilson an...
The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present here the fi...
We present the results ofthe analysis, by means ofthe Wilson-Devinney model offour W UMa-type eclips...
Photoelectric lightcurves of four W UMa systems have been solved using the Wilson-Devinney computer ...
Multicolour lightcurves of three W UMa systems have been solved using the Wilson-Devinney computer c...
Abstract. | The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present ...
Abstract. A photometric analysis of the W UMa sys-tems V 700 Cyg and AW Vir, based on photoelectric ...
A method for the computer synthesis of theoretical light curves and like profiles for close binary s...
CCD photometric observations of a W UMa type contact binary AH Cnc were performed for ten nights fro...
We present light curves and photometric solutions of the contact binary UY UMa in this paper. The li...
The authors have assembled a sample of 42 W Ursae Majoris binary systems (21 W-type, 21 A-type) whos...
In the present study, the activity of the eclipsing binary of the W UMa-type system U Peg is examin...
The α Lyrae-type eclipsing binary AW Cam was observed photoelectrically in three wavelength regions....
We present time-series CCD photometry of AH Cnc, a W UMa–type binary system in the old open cluster ...
Spectroscopic elements of the W UMa system HD 101799 were derived from radial velocity observations....
The UBV photometry of the short period binary FM Vel is analysed by means of the method of Wilson an...
The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present here the fi...
We present the results ofthe analysis, by means ofthe Wilson-Devinney model offour W UMa-type eclips...
Photoelectric lightcurves of four W UMa systems have been solved using the Wilson-Devinney computer ...
Multicolour lightcurves of three W UMa systems have been solved using the Wilson-Devinney computer c...
Abstract. | The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present ...
Abstract. A photometric analysis of the W UMa sys-tems V 700 Cyg and AW Vir, based on photoelectric ...
A method for the computer synthesis of theoretical light curves and like profiles for close binary s...
CCD photometric observations of a W UMa type contact binary AH Cnc were performed for ten nights fro...
We present light curves and photometric solutions of the contact binary UY UMa in this paper. The li...
The authors have assembled a sample of 42 W Ursae Majoris binary systems (21 W-type, 21 A-type) whos...
In the present study, the activity of the eclipsing binary of the W UMa-type system U Peg is examin...
The α Lyrae-type eclipsing binary AW Cam was observed photoelectrically in three wavelength regions....
We present time-series CCD photometry of AH Cnc, a W UMa–type binary system in the old open cluster ...
Spectroscopic elements of the W UMa system HD 101799 were derived from radial velocity observations....
The UBV photometry of the short period binary FM Vel is analysed by means of the method of Wilson an...
The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present here the fi...