Add to ORKGAbstract. Study of eclipsing binaries in open clusters offers information regarding the age of the cluster in addition to the properties of the component stars. In this paper we present the analysis of two W UMa systems discovered in the open cluster Be 33 using the Wilson- Devinney method. 1
Abstract The multicolor photometric observations of the neglected eclipsing binary FT Ursae Majoris ...
In the present study, the activity of the eclipsing binary of the W UMa-type system U Peg is examin...
Abstract We are observing and analyzing changes in the light curves of a few W Ursae Majoris binarie...
Abstract Eclipsing binaries are among the most important sources of information on stellar parameter...
Abstract We present photometric analysis of the two W UMa type binaries identified in the field of d...
Abstract We carried out time-series photometric observations in the Rc-band of the young, poorly stu...
The first photometric solution in the B, V, Rc and Ic filters of the short periodV1833 Ori eclipsing...
Abstract. | The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present ...
WOS: 000343760500006We present the first long-term Johnson UBVR observations and comprehensive photo...
We present the results ofthe analysis, by means ofthe Wilson-Devinney model offour W UMa-type eclips...
We performed new photometric and spectroscopic studies on four W UMa-type eclipsing binaries (V400 L...
Multicolour lightcurves of three W UMa systems have been solved using the Wilson-Devinney computer c...
Aims. The recently discovered eclipsing binary system TYC 2675-663-1 is an X-ray source and shows p...
The authors have assembled a sample of 42 W Ursae Majoris binary systems (21 W-type, 21 A-type) whos...
WOS: 000328373000036Recently, our understanding of the origin of W UMa-type contact binaries has bec...
Abstract The multicolor photometric observations of the neglected eclipsing binary FT Ursae Majoris ...
In the present study, the activity of the eclipsing binary of the W UMa-type system U Peg is examin...
Abstract We are observing and analyzing changes in the light curves of a few W Ursae Majoris binarie...
Abstract Eclipsing binaries are among the most important sources of information on stellar parameter...
Abstract We present photometric analysis of the two W UMa type binaries identified in the field of d...
Abstract We carried out time-series photometric observations in the Rc-band of the young, poorly stu...
The first photometric solution in the B, V, Rc and Ic filters of the short periodV1833 Ori eclipsing...
Abstract. | The W UMa system TU Boo has a period of 0.32438 days and a spectral type G3. We present ...
WOS: 000343760500006We present the first long-term Johnson UBVR observations and comprehensive photo...
We present the results ofthe analysis, by means ofthe Wilson-Devinney model offour W UMa-type eclips...
We performed new photometric and spectroscopic studies on four W UMa-type eclipsing binaries (V400 L...
Multicolour lightcurves of three W UMa systems have been solved using the Wilson-Devinney computer c...
Aims. The recently discovered eclipsing binary system TYC 2675-663-1 is an X-ray source and shows p...
The authors have assembled a sample of 42 W Ursae Majoris binary systems (21 W-type, 21 A-type) whos...
WOS: 000328373000036Recently, our understanding of the origin of W UMa-type contact binaries has bec...
Abstract The multicolor photometric observations of the neglected eclipsing binary FT Ursae Majoris ...
In the present study, the activity of the eclipsing binary of the W UMa-type system U Peg is examin...
Abstract We are observing and analyzing changes in the light curves of a few W Ursae Majoris binarie...