Multicolour lightcurves of three W UMa systems have been solved using the Wilson-Devinney computer code, modified in order to run on a medium-size minicomputer. The solution confirms the contact hypothesis for these systems, one of which lAQ Tue) has turned out to be of Binnendijk's A-type (deeper minimum produced by the eclipse of the more massive star), and the other two (AE Phe and 44 i Boo) of W-type. A comparison with previous solutions is made
In this paper we present a methodology for the solution of binary systems that allows the simultaneo...
The unpublished photoelectric observations of the contact binary W UMa in ultraviolet, blue, and yel...
Abstract. Study of eclipsing binaries in open clusters offers information regarding the age of the c...
Photoelectric lightcurves of four W UMa systems have been solved using the Wilson-Devinney computer ...
We present the results ofthe analysis, by means ofthe Wilson-Devinney model offour W UMa-type eclips...
Abstract. | The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present ...
The authors have assembled a sample of 42 W Ursae Majoris binary systems (21 W-type, 21 A-type) whos...
We present light curves and photometric solutions of the contact binary UY UMa in this paper. The li...
From photoelectric and spectroscopic data available in the literature, we bave determined the elemen...
We present the results of our investigation and first analysis of the geometrical and physical param...
The UBV photometry of the short period binary FM Vel is analysed by means of the method of Wilson an...
Abstract Eclipsing binaries are among the most important sources of information on stellar parameter...
Abstract. A photometric analysis of the W UMa sys-tems V 700 Cyg and AW Vir, based on photoelectric ...
The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present here the fi...
A total of 1088 observations (272 in B,272 in V, 272 in R, and 272 in I) were made from January to F...
In this paper we present a methodology for the solution of binary systems that allows the simultaneo...
The unpublished photoelectric observations of the contact binary W UMa in ultraviolet, blue, and yel...
Abstract. Study of eclipsing binaries in open clusters offers information regarding the age of the c...
Photoelectric lightcurves of four W UMa systems have been solved using the Wilson-Devinney computer ...
We present the results ofthe analysis, by means ofthe Wilson-Devinney model offour W UMa-type eclips...
Abstract. | The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present ...
The authors have assembled a sample of 42 W Ursae Majoris binary systems (21 W-type, 21 A-type) whos...
We present light curves and photometric solutions of the contact binary UY UMa in this paper. The li...
From photoelectric and spectroscopic data available in the literature, we bave determined the elemen...
We present the results of our investigation and first analysis of the geometrical and physical param...
The UBV photometry of the short period binary FM Vel is analysed by means of the method of Wilson an...
Abstract Eclipsing binaries are among the most important sources of information on stellar parameter...
Abstract. A photometric analysis of the W UMa sys-tems V 700 Cyg and AW Vir, based on photoelectric ...
The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present here the fi...
A total of 1088 observations (272 in B,272 in V, 272 in R, and 272 in I) were made from January to F...
In this paper we present a methodology for the solution of binary systems that allows the simultaneo...
The unpublished photoelectric observations of the contact binary W UMa in ultraviolet, blue, and yel...
Abstract. Study of eclipsing binaries in open clusters offers information regarding the age of the c...
Add to ORKG