Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006mnras.366.1289s&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 366, Issue 4, pp. 1289-1294.
Astronomy and Astrophysics
Astronomy
18
Binaries: Eclipsing, Stars: Oscillations, Δ Scuti
Scientific paper
Considering a sample of 20 eclipsing binary systems with δ Scuti type primaries, we discovered that there is a possible relation among the pulsation periods of the primaries and the orbital periods of the systems. According to this empirical relation, the longer the orbital period of a binary, the longer the pulsation period of its pulsating primary. Among the sample, the masses of the secondaries and the separations between the components are known for eight systems for which a logPpuls versus logF (the gravitational pull exerted per gram of the matter on the surface of the primaries by the secondaries) diagram also verifies such an interrelation between the periods. So, as the gravitational force applied by the secondary component onto the pulsating primary increases, its pulsation period decreases. The detailed physics underlying this empirical relation between the periods needs further confirmation, especially theoretically. However, one must also consider the fact that the present sample does not contain a sufficiently large sample of longer period (P > 5 d) binaries.
Akan Can M.
Demircan Osman
Ibanoglu Cafer
Soydugan Esin
Soydugan Faruk
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