Add to ORKGWe present the results ofthe analysis, by means ofthe Wilson-Devinney model offour W UMa-type eclipsing binaries. All four systems result to be of Binnendijk's W-type ; for two of them' (BV Dra and SW Lac) the absolute elements have been computed using the spectroscopic data available in the literature
We present light curves and photometric solutions of the contact binary UY UMa in this paper. The li...
W Ursae Majoris (W UMa)-type variable stars are over-contact eclipsing binary stars. To understand h...
The paper presents new geometric, photometric and absolute parameters, derived from combined spectro...
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...
From photoelectric and spectroscopic data available in the literature, we bave determined the elemen...
Abstract Eclipsing binaries are among the most important sources of information on stellar parameter...
The paper presents new geometric, photometric and absolute parameters, derived from com-bined spectr...
Abstract. Study of eclipsing binaries in open clusters offers information regarding the age of the c...
We performed new photometric and spectroscopic studies on four W UMa-type eclipsing binaries (V400 L...
The authors have assembled a sample of 42 W Ursae Majoris binary systems (21 W-type, 21 A-type) whos...
In this paper we present a methodology for the solution of binary systems that allows the simultaneo...
The UBV photometry of the short period binary FM Vel is analysed by means of the method of Wilson an...
This study is the first attempt to determine the metallicities of W UMa-type binary stars using spec...
Abstract. | The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present ...
We present light curves and photometric solutions of the contact binary UY UMa in this paper. The li...
W Ursae Majoris (W UMa)-type variable stars are over-contact eclipsing binary stars. To understand h...
The paper presents new geometric, photometric and absolute parameters, derived from combined spectro...
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...
From photoelectric and spectroscopic data available in the literature, we bave determined the elemen...
Abstract Eclipsing binaries are among the most important sources of information on stellar parameter...
The paper presents new geometric, photometric and absolute parameters, derived from com-bined spectr...
Abstract. Study of eclipsing binaries in open clusters offers information regarding the age of the c...
We performed new photometric and spectroscopic studies on four W UMa-type eclipsing binaries (V400 L...
The authors have assembled a sample of 42 W Ursae Majoris binary systems (21 W-type, 21 A-type) whos...
In this paper we present a methodology for the solution of binary systems that allows the simultaneo...
The UBV photometry of the short period binary FM Vel is analysed by means of the method of Wilson an...
This study is the first attempt to determine the metallicities of W UMa-type binary stars using spec...
Abstract. | The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present ...
We present light curves and photometric solutions of the contact binary UY UMa in this paper. The li...
W Ursae Majoris (W UMa)-type variable stars are over-contact eclipsing binary stars. To understand h...
The paper presents new geometric, photometric and absolute parameters, derived from combined spectro...