Abstract
The presence of an unseen companion to EV Lac with 2 to 4 Jupiter masses is likely. A period of ~45 years indicates the separation at the time of periastron is ~2 a.u.
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© 1983 Springer Science+Business Media Dordrecht
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Lippincott, S.L. (1983). EV Lacertae: Is Flare Activity Related to an Unseen Planet-Like Companion?. In: Byrne, P.B., Rodonò, M. (eds) Activity in Red-Dwarf Stars. Astrophysics and Space Science Library, vol 102. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7157-8_23
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DOI: https://doi.org/10.1007/978-94-009-7157-8_23
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