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pro vyhledávání: '"Narita, Noria"'
Autor:
Persson, Carina M., Georgieva, Iskra Y., Gandolfi, Davide, Acuña, Lorena, Aguichine, Artem, Muresan, Alexandra, Guenther, Eike, Livingston, John, Collins, Karen A., Fridlund, Malcolm, Goffo, Elisa, Jenkins, James S., Kabáth, Petr, Korth, Judith, Levine, Alan M., Serrano, Luisa M., Vines, José, Barragán, Oscar, Carleo, Ilaria, Colon, Knicole D., Cochran, William D., Christiansen, Jessie L., Deeg, Hans J., Deleuil, Magali, Dragomir, Diana, Esposito, Massimiliamo, Gan, Tianjun, Grziwa, Sascha, Hatzes, Artie P., Hesse, Katharine, Horne, Keith, Jenkins, Jon M., Kielkopf, John F., Klagyivik, P., Lam, Kristine W. F., Latham, David W., Luque, Rafa, Orell-Miquel, Jaume, Mortier, Annelies, Mousis, Olivier, Narita, Noria, Osborne, Hannah L. M., Palle, Enric, Papini, Riccardo, Ricker, George R., Schmerling, Hendrik, Seager, Sara, Stassun, Keivan G., Van Eylen, Vincent, Vanderspek, Roland, Wang, Gavin, Winn, Joshua N., Wohler, Bill, Zambelli, Roberto, Ziegler, Carl
Publikováno v:
A&A 666, A184 (2022)
Highly irradiated planets in the hot Neptune desert are usually either small (R < 2 Rearth) and rocky or they are gas giants with radii of >1 Rjup. Here, we report on the intermediate-sized planet TOI-2196 on a 1.2 day orbit around a G-type star disc
Externí odkaz:
http://arxiv.org/abs/2208.05797