Modeling circumbinary planets: The case of Kepler-38

Wilhelm Kley; Nader Haghighipour

doi:10.1051/0004-6361/201323235

Free Access

Issue		A&A Volume 564, April 2014


Article Number		A72
Number of page(s)		14
Section		Planets and planetary systems
DOI		https://doi.org/10.1051/0004-6361/201323235
Published online		08 April 2014

Online material

Movie 1: The central part of the disk. Locally isothermal Model disk model without a planet, the standard model in the paper, see Fig. 4.

Download Video: Formats: mp4 (1.2 MB) | webm (201.1 KB) | ogg (5.1 MB) | Original mpg (9.0 MB)

Movie 2: Moving planet around binary. Isothermal model: locally isothermal Model disk model with an embedded planet, corresponding to the final phase where the planet is in the 5:1 resonance with the binary, see Fig. 9.

Download Video: Formats: mp4 (1.1 MB) | webm (257.9 KB) | ogg (4.0 MB) | Original mpg (8.0 MB)

Movie 3: Moving planet around binary. Radiative model: radiative disk model with an embedded planet, corresponding to the final phase, of the blue/green curve in Fig. 17.

Download Video: Formats: mp4 (2.5 MB) | webm (339.3 KB) | ogg (12.4 MB) | Original mpg (24.3 MB)

© ESO, 2014

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