Physics
Scientific paper
Jan 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cokon.100..397d&link_type=abstract
Communications of the Konkoly Observatory, No. 100 (Vol. XII, 2), p. 397-406 (1997)
Physics
Scientific paper
The interaction of eclipsing binary star systems with the mass around (in the form of star, planet, envelope or disk) affects the orbital period of these systems. Thus, the long-term orbital period changes of eclipsing binaries which can be deduced by using the observed times of eclipse minima provide a good tool in understanding the interaction of eclipsing binaries with their environment. In the present contribution many examples of the orbital period changes of different eclipsing binaries are presented and interpreted in terms of the interaction with their environment.
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