Zobrazeno 1 - 10
of 224
pro vyhledávání: '"Ibanoglu, C."'
Autor:
Çakırlı, Ö., Ibanoglu, C.
We present new spectroscopic observations of the double-lined eclipsing binary V2653\,Oph. The photometric observations obtained by $ASAS$ were analysed and combined with the analysis of radial velocities for deriving the absolute parameters of the c
Externí odkaz:
http://arxiv.org/abs/1510.02341
We present new spectroscopic observations of the early type, double-lined eclipsing binary V446\,Cep. The radial velocities and the photometric data obtained by $Hipparcos$ were analysed for deriving the astrophysical parameters of the components. Ma
Externí odkaz:
http://arxiv.org/abs/1406.0499
We present new spectroscopic observations of the early type, double-lined eclipsing binary V1441\,Aql. The radial velocities and the available photometric data obtained by $ASAS$ is analysed for deriving the parameters of the components. The componen
Externí odkaz:
http://arxiv.org/abs/1406.0334
We present spectroscopic observations of the massive early type system V745\,Cas, embedded in a multiple star system. The brightest star of the system is the eclipsing binary V745\,Cas with an orbital period of 1.41 days. The radial velocities of bot
Externí odkaz:
http://arxiv.org/abs/1406.0331
We present spectroscopic observations of the massive multiple system HD\,167971, located in the open cluster NGC\,6604. The brighter component of the triple system is the overcontact eclipsing binary MY\,Ser with an orbital period of 3.32\,days. The
Externí odkaz:
http://arxiv.org/abs/1308.4971
BVR light curves and radial velocities for the double-lined eclipsing binary V1135\,Her were obtained. The brighter component of V1135\,Her is a Cepheid variable with a pulsation period of 4.22433$\pm$0.00026 days. The orbital period of the system is
Externí odkaz:
http://arxiv.org/abs/1304.6056
New spectroscopic observations of the double-lined eclipsing binary AQ\,Cas are presented. All available spectroscopic and photometric observations have been analysed for the fundamental properties of the components. Analyses show that the system con
Externí odkaz:
http://arxiv.org/abs/1304.2492
We observed spectroscopically the eclipsing binary system T-Cyg1-01385 in order to determine physical properties of the components. The double-lined nature of the system is revealed for the first time and the radial velocities are obtained for both s
Externí odkaz:
http://arxiv.org/abs/1303.1962
Multi-color light curves and radial velocities for TYC\,1031\,1262\,1 have been obtained and analyzed. TYC\,1031\,1262\,1 includes a Cepheid with a period of 4.15270$\pm$0.00061 days. The orbital period of the system is about 51.2857$\pm$0.0174 days.
Externí odkaz:
http://arxiv.org/abs/1211.1200
Publikováno v:
MNRAS, 2012
The eclipsing binary T-Cyg1-12664 was observed both spectroscopically and photometrically. Radial velocities of both components and ground-based VRI light curves were obtained. The Kepler's R-data and radial velocities for the system were analysed si
Externí odkaz:
http://arxiv.org/abs/1210.8133