Add to ORKGThe UBV photometry of the short period binary FM Vel is analysed by means of the method of Wilson and Devinney. As the spectral type (F8) of the system represents the limit between the A and W sub-classes of contact binaries, both configurations are investigated. The results show that FM Vel has the typical features of the W type of W UMa system. The photometric value of the mass ratio is estimated around 2.0±0.2 and a degree of over-contact of about 16% is found. Both components are thermally coupled.Asociación Argentina de Astronomí
WOS: 000186536600020V1128 Tau is a short period W UMa type eclipsing binary which has a visual compa...
Abstract We carried out time-series photometric observations in the Rc-band of the young, poorly stu...
The W UMa system of ε Coronae Austrinae only shows the spectrum of one of the components which corre...
We present light curves and photometric solutions of the contact binary UY UMa in this paper. The li...
Multicolour lightcurves of three W UMa systems have been solved using the Wilson-Devinney computer c...
Abstract The multicolor photometric observations of the neglected eclipsing binary FT Ursae Majoris ...
The authors have assembled a sample of 42 W Ursae Majoris binary systems (21 W-type, 21 A-type) whos...
This paper presents the results of a combined spectroscopic and photometric study of 20 contact bina...
We present a detailed study of the close eclipsing binary BS Vulpeculae. Although it is relatively b...
Multi-band (B, V and R) photometric and spectroscopic observations of six poorly studied contact bin...
Aims. The recently discovered eclipsing binary system TYC 2675-663-1 is an X-ray source and shows p...
Photoelectric lightcurves of four W UMa systems have been solved using the Wilson-Devinney computer ...
This thesis reports photometric and spectroscopic studies of three close binary systems; BP Velorum,...
This study is focused on the photometric solution of stars of the G2V spectral type. Photometric sol...
We present the results ofthe analysis, by means ofthe Wilson-Devinney model offour W UMa-type eclips...
WOS: 000186536600020V1128 Tau is a short period W UMa type eclipsing binary which has a visual compa...
Abstract We carried out time-series photometric observations in the Rc-band of the young, poorly stu...
The W UMa system of ε Coronae Austrinae only shows the spectrum of one of the components which corre...
We present light curves and photometric solutions of the contact binary UY UMa in this paper. The li...
Multicolour lightcurves of three W UMa systems have been solved using the Wilson-Devinney computer c...
Abstract The multicolor photometric observations of the neglected eclipsing binary FT Ursae Majoris ...
The authors have assembled a sample of 42 W Ursae Majoris binary systems (21 W-type, 21 A-type) whos...
This paper presents the results of a combined spectroscopic and photometric study of 20 contact bina...
We present a detailed study of the close eclipsing binary BS Vulpeculae. Although it is relatively b...
Multi-band (B, V and R) photometric and spectroscopic observations of six poorly studied contact bin...
Aims. The recently discovered eclipsing binary system TYC 2675-663-1 is an X-ray source and shows p...
Photoelectric lightcurves of four W UMa systems have been solved using the Wilson-Devinney computer ...
This thesis reports photometric and spectroscopic studies of three close binary systems; BP Velorum,...
This study is focused on the photometric solution of stars of the G2V spectral type. Photometric sol...
We present the results ofthe analysis, by means ofthe Wilson-Devinney model offour W UMa-type eclips...
WOS: 000186536600020V1128 Tau is a short period W UMa type eclipsing binary which has a visual compa...
Abstract We carried out time-series photometric observations in the Rc-band of the young, poorly stu...
The W UMa system of ε Coronae Austrinae only shows the spectrum of one of the components which corre...