Esposito, M, Covino, E, Desidera, S, Mancini, L, Nascimbeni, V, Sanchez, RZ, Biazzo, K, Lanza, AF, Leto, G, Southworth, J, Bonomo, AS, Mascareno, AS, Boccato, C, Cosentino, R, Claudi, RU, Gratton, R, Maggio, A, Micela, G, Molinari, E, Pagano, I, Piotto, G, Poretti, E, Smareglia, R, Sozzetti, A, Affer, L, Anderson, DR, Andreuzzi, G, Benatti, S, Bignamini, A, Borsa, F, Borsato, L, Ciceri, S, Damasso, M, di Fabrizio, L, Giacobbe, P, Granata, V, Harutyunyan, A, Henning, T, Malavolta, L, Maldonado, J, Fiorenzano, AM, Masiero, S, Molaro, P, Molinaro, M, Pedani, M, Rainer, M, Scandariato, G and Turner, OD (2017) The GAPS Programme with HARPS-N at TNG XIII. The orbital obliquity of three close-in massive planets hosted by dwarf K-type stars: WASP-43, HAT-P-20 and Qatar-2. ASTRONOMY & ASTROPHYSICS, 601. ISSN 1432-0746

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Item Type: Article
Uncontrolled Keywords: planetary systems; Stars: individual: WASP-43; stars: individual: HAT-P-20; Stars: individual: Qatar-2; techniques: radial velocities; techniques: photometrics
Subjects: Q Science > QB Astronomy
?? planetary systems ??
?? stars: individual: HAT-P-20 ??
?? stars: individual: Qatar-2 ??
?? stars: individual: WASP-43 ??
?? techniques: photometric ??
?? techniques: radial velocities ??
Divisions: Faculty of Natural Sciences > School of Chemical and Physical Sciences
Related URLs:
Depositing User: Symplectic
Date Deposited: 04 Jul 2017 08:35
Last Modified: 04 Jul 2017 08:35
URI: http://eprints.keele.ac.uk/id/eprint/3719

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