Could CoRoT-7b and Kepler-10b be remnants of evaporated gas or ice giants?

We present thermal mass loss calculations over evolutionary time scales for the investigation if the smallest transiting rocky exoplanets CoRoT-7b ([Formula: see text]) and Kepler-10b ([Formula: see text]) could be remnants of an initially more massive hydrogen-rich gas giant or a hot Neptune-class...

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Detalles Bibliográficos
Autores principales: Leitzinger, M., Odert, P., Kulikov, Yu.N., Lammer, H., Wuchterl, G., Penz, T., Guarcello, M.G., Micela, G., Khodachenko, M.L., Weingrill, J., Hanslmeier, A., Biernat, H.K., Schneider, J.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Pergamon Press 2011
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3181403/
https://www.ncbi.nlm.nih.gov/pubmed/21969736
http://dx.doi.org/10.1016/j.pss.2011.06.003

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3181403/
https://www.ncbi.nlm.nih.gov/pubmed/21969736
http://dx.doi.org/10.1016/j.pss.2011.06.003

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