Nodal precession of WASP-33b for 11 yr by Doppler tomographic and transit photometric observations

Author(s):
Watanabe, N.; Narita, N.; Palle, E.; Fukui, A.; Kusakabe, N.; Parviainen, H.; Murgas, F.; Casasayas Barris, N.; Johnson, M.C.; Sato, B.; Livingston, J.H.; Leon, J.P. de; Mori, M.; Nishiumi, T.; Terada, Y.; Esparza-Borges, E.; Kawauchi, K.
Published
2022
Publication type
Article / Letter to editor
Techniques - spectroscopicPlanets and satellites - individual - WASP-33bPlanet-star interactionsPlanetary systemsAstrophysics - earth and planetary astrophysics
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2022), Vol. 512, no. 3, p. 4404-4418
hdl
1887/3515365
doi
10.1093/mnras/stac620
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.512.4404W