Meeting on Astrophysics of Variable Stars -- SEP 05-10, 2005 -- Pecs, HUNGARYWOS: 000237451200060We present a photometric study of the overcontact binary AH Cnc. The CCD observations were done with the Russian-Turkish 1.5 m telescope and the light-curve was solved with the Wilson-Devinney code. The physical parameters of the components have been deduced as M-1 = 1.22 M-circle dot, M-2 = 0.20 M-circle dot, R-1 = 1.37 R-circle dot, R-2 = 0.66 R-circle dot, L-1 = 2.65 L-circle dot and L-2 = 0.63 L-circle dot from the obtained orbital parameters and the distance modules of M67. AH Cue ha's been compared with similar systems in the Hertzsprung-Russell diagram.Research Council of the University of LeuvenKU LeuvenKY is supported by the Research Co...
New photometric and spectroscopic solutions of W-type overcontact binary V417 Aql were obtained by s...
WOS: 000305375200001With the aim of providing new and up-to-date absolute parameters of some close b...
Fundamental astrophysical parameters have been derived for Be 45, Be 55, Di 07, Feib 01, Ki 02, NGC ...
Item does not contain fulltextWe present a photometric study of the overcontact binary AH Cnc. The C...
We present time-series CCD photometry of AH Cnc, a W UMa–type binary system in the old open cluster ...
CCD photometric observations of a W UMa type contact binary AH Cnc were performed for ten nights fro...
12 pages, 9 Figures, 13 TablesInternational audienceWe present multi-colour time-series CCD photomet...
We present multi-colour time-series CCD photometry of the solar-age galactic open cluster M 67 (NGC ...
The paper presents combined spectroscopic and photometric orbital solutions for ten close binary sys...
We present multi-colour time-series CCD photometry of the solar-age galactic open cluster M67 (NGC 2...
We present multi-colour time-series CCD photometry of the solar-age galactic open cluster M 67 (NGC ...
New CCD photometry for the eclipsing binary EH Cnc was made from 2009 to 2011, and five new eclipsin...
Wepresent the results of photometrical research of close binary system V859Cyg with possible period...
Abstract CCD photometric observations with B and V passbands were performed on the contact binary V3...
We present four seasons' (2000-2003) ground-based photometry of the short-period contact binary V238...
New photometric and spectroscopic solutions of W-type overcontact binary V417 Aql were obtained by s...
WOS: 000305375200001With the aim of providing new and up-to-date absolute parameters of some close b...
Fundamental astrophysical parameters have been derived for Be 45, Be 55, Di 07, Feib 01, Ki 02, NGC ...
Item does not contain fulltextWe present a photometric study of the overcontact binary AH Cnc. The C...
We present time-series CCD photometry of AH Cnc, a W UMa–type binary system in the old open cluster ...
CCD photometric observations of a W UMa type contact binary AH Cnc were performed for ten nights fro...
12 pages, 9 Figures, 13 TablesInternational audienceWe present multi-colour time-series CCD photomet...
We present multi-colour time-series CCD photometry of the solar-age galactic open cluster M 67 (NGC ...
The paper presents combined spectroscopic and photometric orbital solutions for ten close binary sys...
We present multi-colour time-series CCD photometry of the solar-age galactic open cluster M67 (NGC 2...
We present multi-colour time-series CCD photometry of the solar-age galactic open cluster M 67 (NGC ...
New CCD photometry for the eclipsing binary EH Cnc was made from 2009 to 2011, and five new eclipsin...
Wepresent the results of photometrical research of close binary system V859Cyg with possible period...
Abstract CCD photometric observations with B and V passbands were performed on the contact binary V3...
We present four seasons' (2000-2003) ground-based photometry of the short-period contact binary V238...
New photometric and spectroscopic solutions of W-type overcontact binary V417 Aql were obtained by s...
WOS: 000305375200001With the aim of providing new and up-to-date absolute parameters of some close b...
Fundamental astrophysical parameters have been derived for Be 45, Be 55, Di 07, Feib 01, Ki 02, NGC ...