Different Planetary Eccentricity-period (PEP) Distributions of Small and Giant Planets

We used the database of 1040 short-period (1 ≤ P < 200 days) exoplanets radial-velocity orbits to study the planetary eccentricity-period (PEP) distribution. We first divided the sample into low- and high-mass exoplanet subsamples based on the distribution of the (minimum) planetary masses, which di...

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Detalles Bibliográficos

Autores principales:	Dolev Bashi, Tsevi Mazeh, Simchon Faigler
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	IOP Publishing 2024-01-01
Colección:	The Astronomical Journal
Materias:	Exoplanets Exoplanet dynamics Exoplanet tides Exoplanet evolution Astrostatistics techniques
Acceso en línea:	https://doi.org/10.3847/1538-3881/ad5ffa
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