Short time-scale variability in the light curve of TW Draconis

Warning

This publication doesn't include Institute of Computer Science. It includes Faculty of Science. Official publication website can be found on muni.cz.

Authors	ZEJDA Miloslav MIKULÁŠEK Zdeněk WOLF Marek PEJCHA Ondřej
Year of publication	2006
Type	Article in Periodical
Magazine / Source	Astrophysics and Space Science
MU Faculty or unit	Faculty of Science
Citation
Web	http://adsabs.harvard.edu/abs/2006Ap%26SS.304..161Z
Field	Astronomy and astrophysics
Keywords	Eclipsing binary; short-time variations; TW Dra
Description	We have re-analyzed old photometric UBV data obtained by Papoušek et al. at Skalnaté Pleso, Slovakia (1967 1980) and Brno, Czech Republic (1976 1979) observatories and analyzed new own CCD measurements (Brno, 2003 2005). In both set of photometric data the oscillations in the vicinity of the primary minimum were found. The detected periods are compatible with the previously published ones.
Related projects:	New approaches to variable stars data processing and interpretation Circumstellar envelopes of hot stars Fotometrický výzkum zákrytových dvojhvězd