Obliquities of exoplanet host stars: Nineteen new and updated measurements, and trends in the sample of 205 measurements
Journal article, 2024
Planets and satellites: formation
Planet-star interactions
Planets and satellites: dynamical evolution and stability
Author
Emil Knudstrup
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
Aarhus University
Simon Albrecht
Aarhus University
Princeton University
J. N. Winn
Princeton University
D. Gandolfi
University of Turin
J. J. Zanazzi
University of California
Carina Persson
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
Malcolm Fridlund
Leiden University
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
M. L. Marcussen
Aarhus University
A. Chontos
University of Hawaii
Princeton University
Marcelo Aron Fetzner Keniger
The University of Warwick
N. L. Eisner
Flatiron Institute
Allyson Bieryla
Harvard-Smithsonian Center for Astrophysics
H. Isaacson
University of California
A. W. Howard
California Institute of Technology (Caltech)
L.A. Hirsch
University of Toronto
F. Murgas
University of La Laguna
Instituto de Astrofísica de Canarias
Norio Narita
National Institutes of Natural Sciences
Instituto de Astrofísica de Canarias
University of Tokyo
Enric Palle
University of La Laguna
Instituto de Astrofísica de Canarias
Yugo Kawai
University of Tokyo
D. Baker
Austin College
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 690 A379Subject Categories (SSIF 2011)
Astronomy, Astrophysics and Cosmology
DOI
10.1051/0004-6361/202450627
Related datasets
Additional tables: Obliquities of exoplanet host stars. Nineteen new, updated measurements for the sample of 205 measurements and observed trends [dataset]
DOI: 10.5281/zenodo.13589368