Spin–orbit alignment for KELT-7b and HAT-P-56b via Doppler tomography with TRES

Zhou, George ORCID: https://orcid.org/0000-0002-4891-3517 and Latham, David W. and Bieryla, Allyson and Beatty, Thomas G. and Buchhave, Lars A. and Esquerdo, Gilbert A. and Berlind, Perry and Calkins, Michael L. (2016) Spin–orbit alignment for KELT-7b and HAT-P-56b via Doppler tomography with TRES. Monthly Notices of the Royal Astronomical Society, 460 (3). pp. 3376-3383. ISSN 0035-8711

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Abstract

We present Doppler tomographic analyses for the spectroscopic transits of KELT-7b and HAT-P-56b, two hot-Jupiters orbiting rapidly rotating F-dwarf host stars. These include analyses of archival Tillinghast Reflector Echelle Spectrograph (TRES) observations for KELT-7b, and a new TRES transit observation of HAT-P-56b. We report spin-orbit aligned geometries for KELT-7b (2.7° ± 0.6°) and HAT-P-56b (8° ± 2°). The host stars KELT-7 and HAT-P-56 are among some of the most rapidly rotating planet-hosting stars known. We examine the tidal re-alignment model for the evolution of the spin-orbit angle in the context of the spin rates of these stars. We find no evidence that the rotation rates of KELT-7 and HAT-P-56 have been modified by star-planet tidal interactions, suggesting that the spin-orbit angle of systems around these hot stars may represent their primordial configuration. In fact, KELT-7 and HAT-P-56 are two of three systems in supersynchronous, spin-orbit aligned states, where the rotation periods of the host stars are faster than the orbital periods of the planets.


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Item Type: Article (Commonwealth Reporting Category C)
Refereed: Yes
Item Status: Live Archive
Faculty/School / Institute/Centre: No Faculty
Faculty/School / Institute/Centre: No Faculty
Date Deposited: 01 Feb 2022 02:00
Last Modified: 02 Feb 2022 04:58
Uncontrolled Keywords: Planetary systems; Planets and satellites: individual: (KELT-7b, HAT-P-56b); Astrophysics - Earth and Planetary Astrophysics
Fields of Research (2008): 02 Physical Sciences > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems
Fields of Research (2020): 51 PHYSICAL SCIENCES > 5101 Astronomical sciences > 510109 Stellar astronomy and planetary systems
Socio-Economic Objectives (2008): E Expanding Knowledge > 97 Expanding Knowledge > 970102 Expanding Knowledge in the Physical Sciences
Socio-Economic Objectives (2020): 28 EXPANDING KNOWLEDGE > 2801 Expanding knowledge > 280120 Expanding knowledge in the physical sciences
Identification Number or DOI: https://doi.org/10.1093/mnras/stw1107
URI: http://eprints.usq.edu.au/id/eprint/45052

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