Results 141 to 150 of about 22,639,627 (262)
Solar System Ice Giants: Exoplanets in our Backyard
Future remote sensing of exoplanets will be enhanced by a thorough investigation of our solar system Ice Giants (Neptune-size planets). What can the configuration of the magnetic field tell us (remotely) about the interior, and what implications does that field have for the structure of the magnetosphere; energy input into the atmosphere, and surface ...
Rymer, Abigail +112 more
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Exoplanet mass and radius inferences fundamentally rely on host star mass and radius inferences. Despite the importance of host star mass, radius, and elemental abundance inferences for the derivation of exoplanet internal structure constraints ...
Alejandra Ross +4 more
doaj +1 more source
X-ray Emission from the Exoplanet Hosting LTT 1445 Triple Star System [PDF]
Alexander Brown +7 more
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The Case for Edge-on Binaries: An Avenue Toward Comparative Exoplanet Demographics
Most Sun-like and higher-mass stars reside in systems that include one or more gravitationally bound stellar companions. These systems offer an important probe of planet formation in the most common stellar systems, while also providing key insights into
Joseph E. Hand +2 more
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Exploring and Validating Exoplanet Atmospheric Retrievals with Solar System Analog Observations
Tyler D. Robinson, Arnaud Salvador
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CNO Isotope Ratios Across Exoplanet Systems: Isotope Analysis in Cool Dwarf Exoplanet Hosts
To date, there are still only a handful of dwarf star isotopic abundances in the literature and even fewer of those are from exoplanet host stars. Past isotopic searches have been hindered by limited sensitivity and resolution, strong telluric absorption, and the opacity due to millions of other molecular absorption lines that dominate the observed ...
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It has been suggested that β Pic b has a supersolar metallicity and subsolar C/O ratio. Assuming solar carbon and oxygen abundances for the star β Pic and therefore the planet’s parent protoplanetary disk, β Pic b’s C/O ratio suggests that it formed via ...
Henrique Reggiani +7 more
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White dwarf systems: Exoplanets and debris disks
Although there is abundant and diverse observational evidence in support of white dwarf stars hosting planets or debris disks which form in the catastrophic destruction of various planetary bodies, the key processes that explain these observations are still being intensely investigated.
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VLT/SPHERE survey for exoplanets around young early-type stars, including systems with multi-belt architectures [PDF]
M. Lombart +23 more
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