Photoelectric study of the low-mass semidetached system XX Cephei

Details Photoelectric study of the low-mass semidetached system XX Cephei Photoelectric study of the low-mass semidetached system XX Cephei

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...156...38b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 156, no. 1-2, Feb. 1986, p. 38-50. CNR-supported research.

Astronomy and Astrophysics

Astrophysics

6

Binary Stars, Cepheid Variables, Stellar Mass, Electrophotometry, Stellar Spectrophotometry

Scientific paper

A V and B photoelectric light curve for the eclipsing binary XX Cep is presented and the photometric solution deduced and discussed also from the point of view of the previously assumed semidetached-detached configuration in an eccentric orbit. The system, which is a low-mass one, appears to be normal semidetached with an underluminous subgiant secondary in a circular orbit.

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