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pro vyhledávání: '"Pinte, Ch."'
Autor:
Keppler, M., Penzlin, A., Benisty, M., van Boekel, R., Henning, T., van Holstein, R. G., Kley, W., Garufi, A., Ginski, C., Brandner, W., Bertrang, G. H. -M., Boccaletti, A., de Boer, J., Bonavita, M., Sevilla, S. Brown, Chauvin, G., Dominik, C., Janson, M., Langlois, M., Lodato, G., Maire, A. -L., Ménard, F., Pantin, E., Pinte, Ch., Stolker, T., Szulágyi, J., Thebault, P., Villenave, M., Zurlo, A., Rabou, P., Feautrier, P., Feldt, M., Madec, F., Wildi, F.
Publikováno v:
A&A 639, A62 (2020)
A large fraction of stars is found to be part of binary or higher-order multiple systems. The ubiquity of planets found around single stars raises the question if and how planets in binary systems may form. Protoplanetary disks are the birthplaces of
Externí odkaz:
http://arxiv.org/abs/2005.09037
