Results 181 to 190 of about 5,169,486 (343)
A Possible Hybrid Scenario for Gas Giant Planet Formation in Rings [PDF]
R. H. Durisen +3 more
openalex +1 more source
Multiband Switchable Microwave Absorbing Metamaterials Based on Reconfigurable Kirigami–Origami
A reconfigurable metamaterial featuring tunable microwave‐absorbing and load‐bearing performance is proposed. Stretchable kirigami and bistable origami configurations are integrated as actuating components, and the synergistic deformation mechanisms are systematically analyzed.
Weimin Ding +7 more
wiley +1 more source
Outflow Driven by a Protoplanet Embedded in the TW Hya Disk
Gas giant planets are formed by gas accretion onto planetary cores in protoplanetary disks. However, direct evidence of this process is still lacking, limiting our understanding of planetary formation processes.
Tomohiro C. Yoshida +6 more
doaj +1 more source
A survey of young, nearby, and dusty stars conducted to understand the formation of wide-orbit giant planets [PDF]
Julien Rameau +9 more
openalex +1 more source
The slit height of fluorohectorite 2D‐nanochannels is tuned with Å‐precision (2.4–250 Å). Slit‐height‐dependent ion and water mobilities are quantified by applying EIS, PFG‐NMR, and SFG‐NMR with MD simulations guiding interpretation. Diffuse properties are investigated with CP‐AFM, MD, and PB.
Max Stevenson +11 more
wiley +1 more source
Protoplanetary disks can exhibit asymmetric temperature variations due to phenomena such as shadows cast by the inner disk or localized heating by young planets. We investigate the disk features induced by these asymmetric temperature variations. We find
Zhaohuan Zhu +2 more
doaj +1 more source
Conditions of Inner Planet Formation Inferred From New Estimates of the Sun’s Chemical Composition
Putirka K, Bergemann M, Serenelli A.
europepmc +1 more source
Constraints on terrestrial planet formation timescales and equilibration processes in the Grand Tack scenario from Hf-W isotopic evolution. [PDF]
Zube NG +3 more
europepmc +1 more source
This study presents a novel wide‐bandwidth circularly polarized luminescence (CPL) system combining Cu nanoclusters, perovskite quantum dots, and cholesteric liquid crystals. The design achieves strong CPL emission across 480–750 nm (glum up to 1.31 at 514 nm and 1.46 at 620 nm). Using biomaterials and a simple structure, it offers a promising strategy
Tan‐De Liu +6 more
wiley +1 more source

