Results 31 to 40 of about 828 (196)
Circumbinary planets: migration, trapping in mean-motion resonances, and ejection [PDF]
Context. Most of the planetary systems discovered around binary stars are located at approximately three semi-major axes from the barycentre of their system, curiously close to low-order mean-motion resonances (MMRs).
Emmanuel Gianuzzi +6 more
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Stellar companions to exoplanet host stars: A Lucky Imaging survey of transiting exoplanet systems [PDF]
About half of all nearby stars are part of a binary or multiple star system, yet little is known about how multiplicity affects the formation and subsequent evolution of planetary systems. For instance, stellar companions may promote the inward migration
Wöllert, Maria
core +1 more source
Lithium depletion and the rotational history of exoplanet host stars [PDF]
International audienceContext: It has been reported that exoplanet host stars are lithium depleted compared to solar-type stars without detected massive planets.
Bouvier, J., J. Bouvier, Bouvier, Jerome
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Orbital misalignment of the Neptune-mass exoplanet GJ 436b with the spin of its cool star [PDF]
The angle between the spin of a star and its planets' orbital planes traces the history of the planetary system. Exoplanets orbiting close to cool stars are expected to be on circular, aligned orbits because of strong tidal interactions with the stellar ...
Cegla, H. M. +32 more
core +1 more source
VaTEST I: validation of sub-Saturn exoplanet TOI-181b in narrow orbit from its host star [PDF]
We present here a validation of sub-Saturn exoplanet TOI-181b orbiting a K spectral type star TOI-181 (mass: 0.822 +/- 0.04 M-circle dot, radius: 0.745 +/- 0.02 R-circle dot, temperature: 4994 +/- 50 K) as a part of Validation of Transiting Exoplanets ...
Prasad, Aniket +12 more
core +1 more source
Modeling of Solar-Stellar Connections and the Heliophysics of Exoplanet Systems [PDF]
In the past two and a half decades, advances in the field of exoplanet detection have confirmed more than 4,000 known planets outside of our Solar System \cite{exoplanets}.
Farrish, Alison O.
core
Confirming Resonance in Three Transiting Systems
Although resonant planets have orbital periods near commensurability, resonance is also dictated by other factors, such as the planets’ eccentricities and masses, and therefore must be confirmed through a study of the system’s dynamics.
Tyler Quinn, Mariah G. MacDonald
doaj +1 more source
Peas-in-a-Pod (PIAP) systems have been shown to be common across exoplanet systems, with regular planet spacings and similar planet sizes. In contrast, ultra-short-period planets have displayed distinct differences from PIAP systems, including higher ...
Adam Distler, Juliette Becker
doaj +1 more source
Advancing Heliophysics and Space Weather Modeling Through Open Science
Abstract We present a community‐wide effort to develop a strategy and action plan to advance heliophysics and space weather modeling through open science. While open science has the potential to enhance the quality and pace of scientific discovery, its application to scientific modeling requires more careful consideration regarding open data and open ...
C. Corti +87 more
wiley +1 more source
Records of migration in the exoplanet configurations [PDF]
When compared to our Solar System, many exoplanet systems exhibit quite unusual planet configurations; some of these are hot Jupiters, which orbit their central stars with periods of a few days, others are resonant systems composed of two or more planets
Michtchenko, Tatiana Alexandrovna +2 more
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