Multi-ring structure of the eclipsing disk in EE Cep - possible planets?

C. Galan , M. Mikolajewski , T. Tomov , E. Swierczynski , M. Wiecek , T. Brozek , G. Maciejewski , P. Wychudzki

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M. Hajduk P. T. Rozanski E. Ragan B. Budzisz P. Dobierski S. Frackowiak M. Kurpinska-Winiarska M. Winiarski S. Zola W. Ogloza A. Kuzmicz M. Drozdz E. Kuligowska J. Krzesinski T. Szymanski M. Siwak T. Kundera B. Staels J. Hopkins J. Pye L. Elder G. Myers D. Dimitrov V. Popov E. Semkov S. Peneva D. Kolev I. Iliev I. Barzova I. Stateva N. Tomov S. Dvorak I. Miller L. Brat P. Niarchos A. Liakos K. Gazeas A. Pigulski G. Kopacki A. Narwid A. Majewska M. Steslicki E. Niemczura Y. Ogmen A. Oksanen H. Kucakova T. A. Lister T. A. Heras A. Dapergolas I. Bellas-Velidis R. Kocian A. Majcher

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classification 🌌 astro-ph.SR

keywords diskeclipsingmulti-ringpossiblestructurecampaigneclipsefeatures

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The photometric and spectroscopic observational campaign organized for the 2008/9 eclipse of EE Cep revealed features, which indicate that the eclipsing disk in the EE Cep system has a multi-ring structure. We suggest that the gaps in the disk can be related to the possible planet formation.

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Multi-ring structure of the eclipsing disk in EE Cep - possible planets?

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