Habitability of super-Earth planets around main-sequence stars including red 
giant branch evolution: models based on the integrated system approach

Cuntz, M.; von Bloh, Werner; Schröder, K.-P.; Bounama, C.; Franck, S.

doi:10.1017/S1473550411000280

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Habitability of super-Earth planets around main-sequence stars including red giant branch evolution: models based on the integrated system approach

Authors

Cuntz, M.
Potsdam Institute for Climate Impact Research and Cooperation Partners;

/persons/resource/Werner.von.Bloh

von Bloh, Werner
Potsdam Institute for Climate Impact Research;

Schröder, K.-P.
Potsdam Institute for Climate Impact Research and Cooperation Partners;

Bounama, C.
Potsdam Institute for Climate Impact Research and Cooperation Partners;

Franck, S.
Potsdam Institute for Climate Impact Research and Cooperation Partners;

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Cuntz, M., von Bloh, W., Schröder, K.-P., Bounama, C., Franck, S. (2012): Habitability of super-Earth planets around main-sequence stars including red giant branch evolution: models based on the integrated system approach. - International Journal of Astrobiology, 11, 1, 15-23.
https://doi.org/10.1017/S1473550411000280

Cite as: https://publications.pik-potsdam.de/pubman/item/item_17520

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