A possible misaligned orbit for the young planet AU Mic c

The AU Microscopii planetary system is only 24 Myr old, and its geometry may provide clues about the early dynamical history of planetary systems. Here, we present the first measurement of the Rossiter-McLaughlin effect for the warm sub-Neptune AU Mic c, using two transits observed simultaneously wi...

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Veröffentlicht in:arXiv.org 2024-12
Hauptverfasser: H Yu, Garai, Z, Cretignier, M, Szabó, Gy M, Aigrain, S, Gandolfi, D, Bryant, E M, Correia, A C M, Klein, B, Brandeker, A, Owen, J E, Günther, M N, Winn, J N, Heitzmann, A, Cegla, H M, Wilson, T G, Gill, S, Kriskovics, L, Barragán, O, Boldog, A, Nielsen, L D, Billot, N, Lafarga, M, Meech, A, Alibert, Y, Alonso, R, Bárczy, T, Barrado, D, Barros, S C C, Baumjohann, W, Bayliss, D, Benz, W, Bergomi, M, Borsato, L, Broeg, C, A Collier Cameron, Csizmadia, Sz, Cubillos, P E, Davies, M B, Deleuil, M, Deline, A, Demangeon, O D S, Demory, B O, Derekas, A, Doyle, L, Edwards, B, Egger, J A, Ehrenreich, D, Erikson, A, tier, A, Fossati, L, Fridlund, M, Gazeas, K, Gillon, M, Güdel, M, Isaak, K G, Kiss, L L, Korth, J, Lam, K W F, Laskar, J, A Lecavelier des Etangs, Lendl, M, Magrin, D, Maxted, P F L, McCormac, J, Merín, B, Mordasini, C, Nascimbeni, V, O'Brien, S M, Olofsson, G, Ottensamer, R, Pagano, I, Pallé, E, Peter, G, Piazza, D, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Santos, N C, Scandariato, G, Ségransan, D, Simon, A E, Smith, A M S, Sousa, S G, Southworth, R, Stalport, M, Steinberger, M, Sulis, S, Udry, S, Ulmer, B, Ulmer-Moll, S, V Van Grootel, Venturini, J, Villaver, E, Walton, N A, Wheatley, P J
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