National Repository of Grey Literature 2 records found  Search took 0.00 seconds. 
Doubly-eclipsing systems
Šándorová, Ivana ; Zasche, Petr (advisor) ; Wolf, Marek (referee)
Title: Doubly-eclipsing systems Author: Bc. Ivana Šándorová Institute: Astronomical Institute of Charles University Supervisor: doc. RNDr. Petr Zasche, Ph.D., Astronomical Institute of Charles University Abstract: The study of doubly-eclipsing systems also brings new knowledge about quadru- ple stellar systems as such. And therefore the goal of our work was to create an algorithm for detecting candidates for doubly-eclipsing systems. We had photometric data avail- able from the OGLE project from the Small Magellanic Cloud. After evaluating all the data with our semi-automatic program we selected 74 objects which were further ana- lyzed in PHOEBE. We have obtained 11 new candidates for doubly-eclipsing systems for which we were able to derive both eclipse periods (other 15 candidates in SMC are already known). This gives us only 0.3 % of all binary stars in the SMC for candidates for doubly-eclipsing systems. Out of the 11 new candidates, we detected some variations indicating a common orbit for 6 of them based on the analysis of the O - C diagrams, namely: OGLE SMC-ECL-1086, OGLE SMC-ECL-2339, OGLE SMC-ECL-2515, OGLE SMC-ECL-3075, OGLE SMC-ECL-4756 and OGLE SMC-ECL-6093. Their mutual or- bital period was obtained in the range of 4 to 15 years. This means that these candidates are probably bound 2+2 systems....
Analysis of doubly eclipsing system
van Overloop, Samuel ; Zasche, Petr (advisor) ; Wolf, Marek (referee)
The thesis focuses on selection and analysis of a candidate for a doubly eclipsing system in the Small Magellanic Cloud and on proving its quadruple nature. The OGLE- SMC-ECL-1758 system with periods P1 = 0.92917 d and P2 = 3.73518 d was chosen. The PHOEBE program allowed us to analyse light curves of both eclipsing binaries and determine their parameters such as inclination, surface potencials or the ratio of luminosities. Using these light curves we derived times of eclipses on data from catalogues OGLE II-IV searched for their ETV variations. Thanks to O-C analysis we found proof of relative motion of the two eclipsing binaries around a common centre of mass. Therefore, the OGLE-SMC-ECL-1758 system most probably is a quadruple doubly eclipsing system with a lower limit for its period P = 6021 d. 1

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