The Obliquity of HIP 67522 b: A 17 Myr Old Transiting Hot, Jupiter-sized Planet
A. Heitzmann, Aaron C. Rizzuto(Dairy Australia (Australia)), Andrew Vanderburg(Kavli Institute for Particle Astrophysics and Cosmology), S. C. Marsden(University of Southern Queensland), George Zhou(University of Southern Queensland), Luke G. Bouma(Space Telescope Science Institute), D. J. Wright(University of Southern Queensland), Samuel N. Quinn(Center for Astrophysics Harvard & Smithsonian), P. Petit(Centre National de la Recherche Scientifique), Andrew W. Mann(University of North Carolina at Chapel Hill)
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