TOI-2196 b : rare planet in the hot Neptune desert transiting a G-type star

Autor: Carina M. Persson, Iskra Y. Georgieva, Davide Gandolfi, Lorena Acuna, Artem Aguichine, Alexandra Muresan, Eike Guenther, John Livingston, Karen A. Collins, Fei Dai, Malcolm Fridlund, Elisa Goffo, James S. Jenkins, Petr Kabáth, Judith Korth, Alan M. Levine, Luisa M. Serrano, José Vines, Oscar Barragan, Ilaria Carleo, Knicole D. Colon, William D. Cochran, Jessie L. Christiansen, Hans J. Deeg, Magali Deleuil, Diana Dragomir, Massimiliamo Esposito, Tianjun Gan, Sascha Grziwa, Artie P. Hatzes, Katharine Hesse, Keith Horne, Jon M. Jenkins, John F. Kielkopf, P. Klagyivik, Kristine W. F. Lam, David W. Latham, Rafa Luque, Jaume Orell-Miquel, Annelies Mortier, Olivier Mousis, Noria Narita, Hannah L. M. Osborne, Enric Palle, Riccardo Papini, George R. Ricker, Hendrik Schmerling, Sara Seager, Keivan G. Stassun, Vincent Van Eylen, Roland Vanderspek, Gavin Wang, Joshua N. Winn, Bill Wohler, Roberto Zambelli, Carl Ziegler

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 666, ⟨10.1051/0004-6361/202244118⟩
Astronomy & Astrophysics, 666:A184

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: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3c4e312cc7d86ad0058ed3a743e45c92
https://hdl.handle.net/10023/26356