Results 61 to 70 of about 3,367,182 (237)
ABSTRACT The cytoskeleton of striated muscle integrates force transmission, mechanotransduction, and sarcolemmal stability through coordinated networks of sarcomeres, costameres, and intermediate filaments. Together, these systems establish mechanical continuity between the contractile apparatus, the sarcolemma, and the extracellular matrix.
Houda Cohen +3 more
wiley +1 more source
ABSTRACT We here describe mouse models with complementary homozygous Svil mutations. In skeletal muscle, Svil‐Mut mice express the Svil‐encoded N‐terminus fused to the βgal‐neo gene‐trap tag and lack the highly conserved archvillin C‐terminus; Svil‐KO mice lack expression of all known Svil‐encoded proteins; and Svil‐LoxP mice contain loxP sites for ...
Tara C. Smith +9 more
wiley +1 more source
Eccentric planets constitute a large population of the known exoplanets and may drive significant substructures in protoplanetary disks through planet–disk interactions if their eccentricities are excited early in the planet formation process.
Jiaqing Bi, Min-Kai Lin
doaj +1 more source
Niobium‐Based Chalcogenides as Emerging Electrode Materials for Rechargeable Batteries
This review highlights recent advances in Nb‐based TMCs, covering their structure‐property relationships, synthesis strategies, electrochemical mechanisms, and energy‐storage applications. Emerging approaches including defect engineering, operando characterization, DFT modeling, and AI‐assisted design are discussed to accelerate the development of high‐
Narasimharao Kitchamsetti +3 more
wiley +1 more source
How Eccentric is the Debris Disk of ϵ Eridani? ALMA Reveals a Near-circular Belt
The nearby (3.2 pc) K2V star ϵ Eridani hosts the closest detected debris disk and an exo-Jupiter analog ( ϵ Eridani b). In this work, we reanalyse Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 (1.29 mm) observations of ϵ Eridani to assess
Oto Ulrich +4 more
doaj +1 more source
Environmental interactions in class II systems and their impact on the disk-planet architecture
Context. Protoplanetary disks evolve in clustered environments where interactions with nearby stars and interstellar gas are common. Such environmental processes, including stellar flybys and gas infall, can significantly perturb disk structures over a ...
Poblete Pedro P. +6 more
doaj +1 more source
Planet-disk-wind interaction: The magnetized fate of protoplanets
Context. Models of a planet-disk interaction are mainly based on 2D and 3D viscous hydrodynamic simulations. In such models, accretion is classically prescribed by an αv parameter which characterizes the turbulent radial transport of angular momentum in ...
Wafflard-Fernandez, Gaylor +3 more
core +1 more source
The NGB additive can concurrently address anode and cathode issues during Zn‐Mn battery cycling by constructing a hierarchical interfacial layer on the anode surface to alleviate side reactions and modulate zinc deposition and by incorporating Fe3+ ions into the α‐MnO2 cathode to improve its structural stability and electrical conductivity.
Xiaoliang Zhang +7 more
wiley +1 more source
Nickel‐Catalyzed LiF‐Rich Interface for Silicon Anodes
Modulating the decomposition of F‐containing species in the electrolyte to form LiF‐rich SEI has been proven to be an effective strategy for interface optimization. Herein, through nickel‐catalyzed pyrolysis of carbon precursors on silicon, graphene‐like carbon was formed to construct three‐dimensional conductive networks.
Haoqi Li +13 more
wiley +1 more source
Concertos of planet-disk interactions: thermal and kinematic fingerprints [PDF]
Planets form in protoplanetary disks, where interactions with their natal environments shape disk evolution and leave observable signatures. High-resolution observations over the past decade have revealed substructures such as gaps, rings, and non ...
Chen, Kan
core +1 more source

