The GAPS programme with HARPS-N at TNG: XVI. Measurement of the Rossiter–McLaughlin effect of transiting planetary systems HAT-P-3, HAT-P-12, HAT-P-22, WASP-39, and WASP-60

Luigi Mancini,M. Esposito,E. Covino,John Southworth,K. Biazzo,I. Bruni,Simona Ciceri,Dafydd W. Evans,A. F. Lanza,E. Poretti,Paula Sarkis,Alexis M. S. Smith,Matteo Brogi,Laura Affer,Serena Benatti,Andrea Bignamini,C. Boccato,A. S. Bonomo,F. Borsa,I. Carleo,Riccardo Claudi,R. Cosentino,Mario Damasso,Silvano Desidera,P. Giacobbe,E. González-Álvarez,Raffaele Gratton,A. Harutyunyan,G. Leto,A. Maggio,Luca Malavolta,J. Maldonado,A. Martinez-Fiorenzano,S. Masiero,Giuseppina Micela,E. Molinari,Valerio Nascimbeni,Isabella Pagano,M. Pedani,Giampaolo Piotto,M. Rainer,G. Scandariato,Riccardo Smareglia,Alessandro Sozzetti,Gloria Andreuzzi,Th. Henning

The GAPS programme with HARPS-N at TNG: XVI. Measurement of the Rossiter–McLaughlin effect of transiting planetary systems HAT-P-3, HAT-P-12, HAT-P-22, WASP-39, and WASP-60

2018

Context. The measurement of the orbital obliquity of hot Jupiters with different physical characteristics can provide clues to the mechanisms of migration and orbital evolution of this particular c ...

Keywords:

Planetary system
Rossiter–McLaughlin effect
Astrophysics
Physics

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