Abstract
GW Ori is a single line spectroscopic binary CTTS with orbital period P ≃ 242d and nearly circular (e < 0.05) orbits of the companions (Mathieu et al.1991). Radius of the primary according to these authors is Ri ≃ 5.6 R⨀.
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© 1999 Springer Science+Business Media Dordrecht
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Lamzin, S., Shevchenko, V., Grankin, K., Melnikov, S. (1999). On the Eclipses in GW Ori Double System. In: Lago, M.T.V.T., Blanchard, A. (eds) The Non-Sleeping Universe. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4497-1_40
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DOI: https://doi.org/10.1007/978-94-011-4497-1_40
Publisher Name: Springer, Dordrecht
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