Light Curve and Orbital Elements of V 337 Aquilae

Details Light Curve and Orbital Elements of V 337 Aquilae Light Curve and Orbital Elements of V 337 Aquilae

May 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..11..232c&link_type=abstract

Astrophysics and Space Science, Volume 11, Issue 2, pp.232-243

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

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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