Results 71 to 80 of about 34,106 (228)
Heat conduction has been found a plausible solution to explain discrepancies between expected and measured temperatures in hot bubbles of planetary nebulae (PNe).
Rühling, Ute +3 more
core +1 more source
A Computational Workflow for Cell Line Profiling by Imaging Mass Cytometry
ABSTRACT In single‐cell spatial phenotyping biology, imaging mass cytometry (IMC) stands out as a cutting‐edge, highly multiplexed technology driving discoveries across various disease areas. In vitro profiling relies on tumor‐derived cancer cell lines, known for their diverse morphologies and phenotypes.
Alexandre Bouzekri +2 more
wiley +1 more source
The impact of grain orientation and surface temperature on helium bubble growth at tungsten surfaces exposed to low-pressure helium plasmas was investigated by analyzing the nanoholes formed at the surface.
Mounir Alfazzaa +5 more
doaj +1 more source
Sonoluminescence: Nature's Smallest BlackBody
The Spectrum of the light emitted by a sonoluminescing bubble is extremely well fit by the spectrum of a blackbody. Furthermore the radius of emission can be smaller than the wavelength of the light.
Baltes +26 more
core +1 more source
The Pangkaimen Au–Ag deposits belong to the epithermal Au deposits, which are of great significance for guiding the research and development of this type of gold deposit. Metallogenic model diagram of Pangkaimen Au–Ag deposit. ABSTRACT The gold (Au) metallogenic belt in the northern Great Xing'an Range is characterised by the wide occurrence of the ...
Sheng Lu +8 more
wiley +1 more source
Carbonates from Santos Basin revealed U–Pb ages correlated with basalt ages (A), suggesting that they were formed during magmatic events. These events placed hot CO2 in the reservoir, which, when mixed with carbonate‐rich cold water (B), led to thermal convection, enabling the formation of the U contained in the carbonates.
Marco António Ruivo de Castro e Brito +8 more
wiley +1 more source
X-rays and hard UV radiation From the First Galaxies: Ionization Bubbles and 21 cm Observations
The first stars and quasars are known sources of hard ionizing radiation in the first billion years of the Universe. We examine the joint effects of X-rays and hard UV radiation from such first-light sources on the hydrogen and helium reionization of the
Aldrovandi +79 more
core +1 more source
DBDI enables real‐time analysis of volatile terpenes and generates atmosphere‐dependent reagent ions that produce structure‐specific spectral patterns. By tuning humidity or dopant gases, DBDI‐MS differentiates terpene isomers that appear identical by EI.
Justine Raeber +4 more
wiley +1 more source
Probing Strongly Coupled Chameleons with Slow Neutrons
We consider different methods to probe chameleons with slow neutrons. Chameleon modify the potential of bouncing neutrons over a flat mirror in the terrestrial gravitational field.
Brax, Philippe +2 more
core +3 more sources

