Results 181 to 190 of about 4,018,158 (274)
In this study, heterosite FePO4 is obtained by chemical delithiation of LiFePO4 using O2. The extracted lithium source is recovered as lithium acetate, and the obtained FePO4 is used as an electrode for the charged‐state lithium metal battery (lean Li/FePO4 configuration), which shows stable cycling performance compared to the conventional lithium ...
Fumiyasu Nozaki+2 more
wiley +1 more source
Planetary atmospheres Through Time: Effects of Mass Loss and Thermal Evolution [PDF]
Atmospheric mass loss is a fundamental phenomenon shaping the structure and evolution of planetary atmospheres. It can engage processes ranging from global interactions with the host star and large-scale hydrodynamic outflows to essentially microphysical kinetic effects.
arxiv
Hydrogen lines from forming planets are crucial for understanding planet formation. However, the number of planetary hydrogen line detections is still limited. Recent JWST/NIRSpec observations have detected Paschen and Brackett hydrogen lines at TWA 27 B
Yuhiko Aoyama+2 more
doaj +1 more source
Stable mass ranges of ν Andromedae planetary system [PDF]
Takashi Itô, Shoken M. Miyama
openalex +1 more source
Differences between Stable and Unstable Architectures of Compact Planetary Systems
We present a stability analysis of a large set of simulated planetary systems of three or more planets based on architectures of multiplanet systems discovered by Kepler and K2.
Kathryn Volk, Renu Malhotra
doaj +1 more source
Discovery of a Planetary-Mass Brown Dwarf with a Circumstellar Disk [PDF]
K. L. Luhman+6 more
openalex +1 more source
The T Tauri Phase Down to Nearly Planetary Masses: Echelle Spectra of 82 Very Low Mass Stars and Brown Dwarfs [PDF]
Subhanjoy Mohanty+2 more
openalex +1 more source
The article introduces WACEfNet, a new convolutional neural network architecture optimized for efficient aerial image analysis under resource constraints. It creatively integrates attention mechanisms and atrous convolutions into a compact widened residual network framework.
Md Meftahul Ferdaus+4 more
wiley +1 more source
COJ= 2–1 and 4–3 Observations of Proto–planetary Nebulae: Time‐variable Mass Loss [PDF]
Bruce J. Hrivnak, John H. Bieging
openalex +1 more source