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How eclipse time variations, eclipse duration variations and radial velocities can reveal S-type planets in close eclipsing binaries

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Heller,  René
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;

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Oshagh, M., Heller, R., & Dreizler, S. (2016). How eclipse time variations, eclipse duration variations and radial velocities can reveal S-type planets in close eclipsing binaries. Mon. Not. Roy. Astron. Soc., 466, 4683-4691. doi:10.1093/mnras/stw3313.


Cite as: http://hdl.handle.net/11858/00-001M-0000-002D-ED7B-6
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