[HTML][HTML] Stellar obliquities in exoplanetary systems
SH Albrecht, RI Dawson, JN Winn - Publications of the …, 2022 - iopscience.iop.org
The rotation of a star and the revolutions of its planets are not necessarily aligned. This
article reviews the measurement techniques, key findings, and theoretical interpretations …
article reviews the measurement techniques, key findings, and theoretical interpretations …
Origins of hot Jupiters
RI Dawson, JA Johnson - Annual Review of Astronomy and …, 2018 - annualreviews.org
Hot Jupiters were the first exoplanets to be discovered around main sequence stars and
astonished us with their close-in orbits. They are a prime example of how exoplanets have …
astonished us with their close-in orbits. They are a prime example of how exoplanets have …
The origin and evolution of multiple star systems
SSR Offner, M Moe, KM Kratter, SI Sadavoy… - arXiv preprint arXiv …, 2022 - arxiv.org
Observational advances over the last decade have enabled high-resolution, interferometric
studies of forming multiple systems, statistical surveys of multiplicity in star-forming regions …
studies of forming multiple systems, statistical surveys of multiplicity in star-forming regions …
SOAR TESS survey. I. Sculpting of TESS planetary systems by stellar companions
Abstract The Transiting Exoplanet Survey Satellite (TESS) is finding transiting planet
candidates around bright, nearby stars across the entire sky. The large field of view …
candidates around bright, nearby stars across the entire sky. The large field of view …
Hot Jupiters: origins, structure, atmospheres
JJ Fortney, RI Dawson… - Journal of Geophysical …, 2021 - Wiley Online Library
We provide a brief review of many aspects of the planetary physics of hot Jupiters. Our aim is
to cover most of the major areas of current study while providing the reader with additional …
to cover most of the major areas of current study while providing the reader with additional …
Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets
J Drazkowska, B Bitsch, M Lambrechts… - arXiv preprint arXiv …, 2022 - arxiv.org
Our understanding of planet formation has been rapidly evolving in recent years. The
classical planet formation theory, developed when the only known planetary system was our …
classical planet formation theory, developed when the only known planetary system was our …
The occurrence rate of giant planets orbiting low-mass stars with TESS
We present a systematic search for transiting giant planets () orbiting nearby low-mass stars
(). The formation of giant planets around low-mass stars is predicted to be rare by the core …
(). The formation of giant planets around low-mass stars is predicted to be rare by the core …
The Upper Edge of the Neptune Desert Is Stable Against Photoevaporation
S Vissapragada, HA Knutson… - The Astronomical …, 2022 - iopscience.iop.org
Transit surveys indicate that there is a deficit of Neptune-sized planets on close-in orbits. If
this" Neptune desert" is entirely cleared out by atmospheric mass loss, then planets at its …
this" Neptune desert" is entirely cleared out by atmospheric mass loss, then planets at its …
Exoplanet statistics and theoretical implications
In the past few years, significant advances have been made in understanding the
distributions of exoplanet populations and the architecture of planetary systems. We review …
distributions of exoplanet populations and the architecture of planetary systems. We review …
Unresolved stellar companions with Gaia DR2 astrometry
V Belokurov, Z Penoyre, S Oh, G Iorio… - Monthly Notices of …, 2020 - academic.oup.com
For stars with unresolved companions, motions of the centre of light and that of mass
decouple, causing a single-source astrometric model to perform poorly. We show that such …
decouple, causing a single-source astrometric model to perform poorly. We show that such …