Analysis on the photometric orbit of DI Pegasi

Details Analysis on the photometric orbit of DI Pegasi Analysis on the photometric orbit of DI Pegasi

Dec 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968jkas....1....1c&link_type=abstract

Journal of the Korean Astronomical Society, vol. 1, no. 1, p. 1-18

Astronomy and Astrophysics

Astronomy

Scientific paper

The photometric orbital elements of an Algol-type eclipsing variable, DI Pegasi, are derived by means of Fourier transforms from two-color photoelectric observations. The system shows a long term variation of its orbital period, which is interpreted as due to a continuing mass loss mechanism from the secondary component. Physical dimensions and model of the system are also suggested here

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