Esposito, M and Covino, E and Desidera, S and Mancini, L and Nascimbeni, V and Sanchez, RZ and Biazzo, K and Lanza, AF and Leto, G and Southworth, J and Bonomo, AS and Mascareno, AS and Boccato, C and Cosentino, R and Claudi, RU and Gratton, R and Maggio, A and Micela, G and Molinari, E and Pagano, I and Piotto, G and Poretti, E and Smareglia, R and Sozzetti, A and Affer, L and Anderson, DR and Andreuzzi, G and Benatti, S and Bignamini, A and Borsa, F and Borsato, L and Ciceri, S and Damasso, M and di Fabrizio, L and Giacobbe, P and Granata, V and Harutyunyan, A and Henning, T and Malavolta, L and Maldonado, J and Fiorenzano, AM and Masiero, S and Molaro, P and Molinaro, M and Pedani, M and Rainer, M and 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

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