Photometric observations of two very long period eclipsing binaries: AZ Cas and EE Cep

Details Photometric observations of two very long period eclipsing binaries: AZ Cas and EE Cep Photometric observations of two very long period eclipsing binaries: AZ Cas and EE Cep

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..318..378m&link_type=abstract

In Spectroscopically and Spatially Resolving the Components of the Close Binary Stars, Proceedings of the Workshop held 20-24 Oc

Astronomy and Astrophysics

Astronomy

Scientific paper

This paper reports new photometric observations of minima of two very long-period eclipsing systems: AZ Cas (P=3402 °}) and EE Cep (P=2050 °). In order to match the observed depth of the primary minimum of AZ Cas we had to introduce a third light component. For EE Cep, the shape of the eclipse can be explained by a model that includes a dark precessing disk in the system.

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