Results 81 to 90 of about 4,499,156 (300)
The Vertical and Adiabatic Ionization Energies of Silicon Carbide Clusters, (SiC)n, With n = 1–12
Frontiers in Astronomy and Space Sciences, 2021 David Gobrecht
doaj +1 more source
FEBS Open Bio, EarlyView.KDAC6 has been associated with cell motility and actin structures, but specific domain contributions are not established. The two catalytic domains have differential effects on motility and F‐actin regulation, affecting cortical F‐actin density, motility, stress fibers, and cell spreading.
Taylor V. Joseph +7 more
wiley +1 more source
Cosmological galaxy formation simulations with dust
, 2016 Recent observations of galaxies in the redshift range 6.5 < z < 7.5 show an increasing evidence of a significant amount of dust ([1],[2],[3]). Intepreting the role of different stellar populations, their formation rates and the various phases of ...
LUCA GRAZIANI +2 more
core
Accurate and noninvasive prostate cancer detection using plasma‐derived extracellular vesicle RNA
FEBS Open Bio, EarlyView.Plasma extracellular vesicles were captured with WGA‐conjugated magnetic beads and profiled for RNA biomarkers. A three‐RNA panel (NM_024955, NR_047469, and NR_002564) distinguished prostate cancer from healthy controls and benign prostatic hyperplasia, supporting a simple, noninvasive approach to improve prostate cancer detection.
Hanping Wei, Haoran Wu, Wei Feng
wiley +1 more source
Dust Clumping in Outer Protoplanetary Disks: The Interplay among Four Instabilities
The Astrophysical Journal LettersDust concentration in protoplanetary disks (PPDs) is the first step toward planetesimal formation, a crucial yet highly uncertain stage in planet formation.
Pinghui Huang, Xue-Ning Bai
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Dust evolution across cosmic times as seen through DUSTY-GAEA
Astronomy & AstrophysicsFor many decades, dust has been recognised as an important ingredient in galaxy formation and evolution. This paper presents a novel self-consistent implementation of dust formation by stars, destruction by supernova shocks and hot gas, and growth within
Osman Omima +4 more
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The Astronomical Journal, 1977 Scaling from the observed time of dust formation in Nova FH Ser 1970 and using plausible assumptions for the postmaximum luminosities of novae, the time scale for observable dust to form in novae is t/sub d/approx. = (320/v) (L/L/sub sun/)/sup 1///sup 2/ days, where v is the expansion velocity in kilometers/sec. The predicted t/sub d/ are in reasonable
openaire +1 more source
Molecular catastrophes and the formation of circumstellar dust [PDF]
Symposium - International Astronomical Union, 1987 Radiative instabilities due to simple molecules may convert chromospheric material into masering molecules and dust capable of being removed from the star by radiation pressure.
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FEBS Open Bio, EarlyView.Biophysical characterisation shows that NanX, a membrane transport protein from the major facilitator superfamily (MFS), forms both monomers and dimers after purification. AlphaFold modelling and substrate docking provide information on residues likely involved in substrate recognition for NanX and another MFS member, NanT.
Michael C. Newton‐Vesty +13 more
wiley +1 more source
Understanding the effects of sand and dust accumulation on photovoltaic modules [PDF]
, 2012 Numerical and analytical models of sand and dust particle accumulation on photovoltaic modules in dry regions are presented and supported by a laboratory investigation of sand particle accumulation on a glass surface.
Moir, Robert +5 more
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