Results 191 to 200 of about 5,169,486 (343)
exoALMA. III. Line-intensity Modeling and System Property Extraction from Protoplanetary Disks
The ALMA large program exoALMA offers a unique window into the three-dimensional physical and dynamical properties of 15 circumstellar disks where planets may be actively forming. Here, we present an analysis methodology to map the gas disk structure and
Andrés F. Izquierdo +39 more
doaj +1 more source
Gd‐doped BFO (BGFO) exhibits a ∼2‐order reduction in leakage current owing to its lowest content of oxygen vacancies. This leads to a ∼2.5‐fold increase in remnant polarization. These improvements in BGFO effectively boost charge separation and transportation, resulting in the greatest incident photon‐to‐current efficiency of 12.9 ± 0.73% and a ∼1.5 ...
Ming‐Wei Chu +7 more
wiley +1 more source
Particle Accretion in Microgravity. I. Particle Sizes and Bulk Densities
The precise mechanisms related to the accretion of protoplanetesimals from dust in protoplanetary disks (PPDs) are poorly understood. In order to better understand the early stages of planet formation and the growth of millimeter–centimeter agglomerates,
Akbar D. Whizin +3 more
doaj +1 more source
Radial Distribution of Planets. Predictions based on the Core Accretion Gas Capture Planet formation Model [PDF]
K. Kornet, S. Wolf
openalex +1 more source
A Termite‐Inspired Alternative to Cement
A termite‐inspired composite of clay, cellulose, and lignin forms a dense fibrous network with concrete‐like strength (32 MPa) and superior elasticity, processed at ambient temperature. Abstract Clay combined with organic materials is used by termites as a strong and durable construction material for their mounds with minimal environmental impact. Here,
Oren Regev +3 more
wiley +1 more source
Mid-infrared Spectrum of the Disk around the Forming Companion GQ Lup B Revealed by JWST/MIRI
GQ Lup B is a forming brown dwarf companion ( M ∼ 10–30 M _J ) showing evidence for an infrared excess associated with a disk surrounding the companion itself.
Gabriele Cugno +7 more
doaj +1 more source
Chapter 22. Primordial Atmosphere Surrounding a Protoplanet and Formation of Jovian Planets [PDF]
Hiroshi Mizuno, Kiyoshi Nakazawa
openalex +1 more source
This study explores a cost‐effective alternative by incorporating oxophilic dopants into non‐precious metal hosts to enhance water dissociation and catalyst stability. Computational screening identified Ni─V, Ni─Mo, and Co─V as top candidates. Subsequent experiments confirmed Ni20V exhibits superior HER activity, achieving 76 mV lower overpotential ...
Hyeonjung Jung +13 more
wiley +1 more source
Radial Gradients in Dust Opacity Lead to Preferred Region for Giant Planet Formation
Yayaati Chachan +2 more
openalex +1 more source
DID PLANET FORMATION BEGIN INSIDE PERSISTENT GASEOUS VORTICES? [PDF]
P. Barge, Joël Sommeria
openalex +1 more source

