Results 151 to 160 of about 5,220,245 (377)
Highly Selective Toward HER or CO2RR by Regulating Cu Single and Dual Atoms on g‐C3N4
This systematic study provides insights into the design of electrocatalysts for hydrogen evolution reaction (HER) and carbon dioxide reduction (CO2RR). It serves as a useful guide for tuning catalyst architecture toward efficient multifunctional performance by varying synthetic parameters, demonstrating the impact of copper (Cu) species ranging from ...
Wan‐Ting Chen +9 more
wiley +1 more source
We present the Atacama Large Millimeter/submillimeter Array Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO), a large program of the ALMA. AGE-PRO aims to systematically trace the evolution of gas disk mass and size throughout the lifetime of ...
Ke Zhang +21 more
doaj +1 more source
Towards the Rosetta Stone of planet formation
Transiting exoplanets (TEPs) observed just ~10 Myrs after formation of their host systems may serve as the Rosetta Stone for planet formation theories. They would give strong constraints on several aspects of planet formation, e.g.
Schmidt T.O.B. +20 more
doaj +1 more source
Disk-Planet Interactions During Planet Formation
14 pages, 14 figures, to appear in "Protostars and Planets V". A version with high resolution figures is available from http://www.maths.qmul.ac.uk/~rpn/preprints/index ...
Papaloizou, J. C. B. +4 more
openaire +2 more sources
Thermal Phase‐Modulation of Thickness‐Dependent CVD‐Grown 2D In2Se3
A comprehensive study of CVD‐grown 2D In2Se3 reveals a distinct thickness‐dependent phase landscape and a reversible, thermally driven transformation between β″ and β* variants. In situ TEM electron diffraction and Raman spectroscopy reveal structural dynamics, while the structural invariance of the α‐phase in ultrathin regimes highlights its stability—
Dasun P. W. Guruge +6 more
wiley +1 more source
Broadening the Canonical Picture of EUV-driven Photoevaporation of Accretion Disks
Photoevaporation driven by hydrogen-ionizing extreme-ultraviolet (EUV) radiation profoundly shapes the lives of diverse astrophysical objects. We construct an analytical model accounting for the finite timescales of photoheating and photoionization and ...
Riouhei Nakatani +2 more
doaj +1 more source
Tidal dissipation and the formation ofKeplernear-resonant planets [PDF]
J.-B. Delisle, J. Laskar
openalex +1 more source
Anisometric carbon nanodots are synthesized directly from a liquid crystal precursor and embedded into polymer network liquid crystals to create soft, multifunctional photonic films. These hybrid devices exhibit polarized photoluminescence, broad UV absorption, and fast, electrically tunable light modulation.
Mangesh D. Patekari +4 more
wiley +1 more source
Dust Rings as a Footprint of Planet Formation in a Protoplanetary Disk [PDF]
Kazuhiro Kanagawa +2 more
openalex +1 more source
Giant Planet Formation by Core Accretion
We present a review of the standard paradigm for giant planet formation, the core accretion theory. After an overview of the basic concepts of this model, results of the original implementation are discussed.
Alibert, Yann +3 more
core

