The Semi-detached system RT Persei and its light curve

Details The Semi-detached system RT Persei and its light curve The Semi-detached system RT Persei and its light curve

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..47..277m&link_type=abstract

Astrophysics and Space Science, vol. 47, Apr. 1977, p. 277-298. Research supported by the Consiglio Nazionale delle Richerche.

Astronomy and Astrophysics

Astrophysics

15

Astronomical Models, Eclipsing Binary Stars, Light Curve, Periodic Variations, Orbit Calculation, Tables (Data)

Scientific paper

The observed V light curve of the eclipsing binary RT Persei has been analyzed by four different methods of solution to obtain the geometrical and photometric elements of the system. The results show good agreement within about 6%. The system exhibits a variable light curve, and a tentative hypothesis is made to explain this behavior by considering a dynamical instability that may be responsible for matter circulation through the system as well as for the variability of the period.

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