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
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DOI: 10.1051/0004-6361/201629720
Abstract: Context. The orbital obliquity of planets with respect to the rotational axis of their host stars is a relevant parameter for the characterization of the global architecture of planetary systems and a key observational constraint… read more here.
Keywords: dwarf type; wasp hat; obliquity; hat qatar ... See more keywords