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Light curve and orbital elements of V 337 Aquilae

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Abstract

From photoelectric observations of V 337 Aql a new solution is carried out. Transit at primary eclipse in disagreement with the Wright-Dugan results is found. Both Russell-Merrill and Kitamura methods of light curve solution are used. The slight period variation and the distortions of the light curve would support the idea that a mass exchange could be in act.

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Authors and Affiliations

  1. Osservatorio Astrofisico Catania, Università degli Studi di Catania, Consiglio Nazionale delle Ricerche, Catania, Italy

    F. A. Catalano, S. Catalano & M. Rodonò

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  1. F. A. Catalano
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  2. S. Catalano
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  3. M. Rodonò
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Catalano, F.A., Catalano, S. & Rodonò, M. Light curve and orbital elements of V 337 Aquilae. Astrophys Space Sci 11, 232–243 (1971). https://doi.org/10.1007/BF00661356

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