Results 81 to 90 of about 7,212 (309)
The Epoch of Giant Planet Migration Planet Search Program. I. Near-infrared Radial Velocity Jitter of Young Sun-like Stars [PDF]
Quang H. Tran +10 more
openalex +1 more source
Corporate Involvement in the Sustainable Development Goals: The Case of Banks in Sub‐Saharan Africa
ABSTRACT This study examines the extent of banks' involvement in the Sustainable Development Goals (SDGs) and factors influencing their participation in Sub‐Saharan Africa (SSA). Previous studies have highlighted the dearth of research conducted in developing countries.
Adwoa Appiah +4 more
wiley +1 more source
On the Exoplanet Yield of Gaia Astrometry
We reexamine the expected yield of Gaia astrometric planet detections using updated models for giant-planet occurrence, the local stellar population, and Gaia’s demonstrated astrometric precision. Our analysis combines a semianalytic model that clarifies
Caleb Lammers, Joshua N. Winn
doaj +1 more source
Terrestrial planet formation during giant planet formation and giant planet migration
Context. Terrestrial planet formation (TPF) is a difficult problem that has vexed researchers for decades. Numerical models are only partially successful at reproducing the orbital architecture of the inner planets, but have generally not considered the effect of the growth of the giant planets.
openaire +1 more source
ABSTRACT Championed as a pathway for sustainable growth, the “blue economy” (BE) has garnered increasing interest in recent decades. International organizations like the World Bank and the Organization for Economic Cooperation and Development (OECD) increasingly point to marine resources and activities as a “new frontier” for economic growth ...
Flora St. Pier +2 more
wiley +1 more source
Astrometric positions for 18 irregular satellites of giant planets from 23 years of observations [PDF]
A. R. Gomes-Júnior +14 more
openalex +1 more source
Formation of Giant Planets [PDF]
This is a descriptive and non‐mathematical summary of giant planet formation theories. There are two end‐member models, core accretion and disk instability. In the core accretion model, several to ten Earth masses of solid (ice and rock) accumulate and this promotes subsequent gas accretion.
openaire +2 more sources
Multimetal Doping and Heterostructure Engineering of RuO2 for Durable and Efficient Oxygen Evolution
A MnCoNi–RuO2 heterostructure engineered through multimetal doping and mixed‐oxide interface formation generates lattice distortion, oxygen vacancies, and electronically optimized active sites for the oxygen evolution reaction. MnCoNi–RuO2 achieves high activity and durability across alkaline and acidic media, sustaining 100 h (AEMWE) anion exchange ...
Md. Mofakkharulhashan +5 more
wiley +1 more source
Accretion of ice giant planets from massive protoplanets whose migration is blocked by Jupiter and Saturn [PDF]
G. Benedetti-Rossi +4 more
openalex +1 more source
Drones equipped with thermal infrared (TIR) cameras offer significant time and labor savings in estimating wild ungulate populations. However, accurately monitoring forest‐dwelling ungulates remains challenging due to their elusive behavior and complex habitat.
Jinhwi Kim, Donggul Woo
wiley +1 more source

