Results 131 to 140 of about 4,003,229 (276)
Formation and Evolution of Young Massive Clusters
, 2006 to be published in "Mass loss from stars and the evolution of stellar clusters," eds. A. de Koter, L. Smith, R. Waters, ASP Conf. Ser.
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Advanced Science, EarlyView.CDegSR, a new tool for imaging RNA at single molecule level in living cells was developed by researchers. Background noise was eliminated by protein engineering and making it degrade when not bound to its target. This allowed individual RNA molecules to be clearly imaged and tracked.
Shipeng Shao, Hongchen Zhang
wiley +1 more source
Multiwavelength study of the Carina–Sagittarius Arm
Astronomy & AstrophysicsAims. Our main goal is to determine whether the lower stellar density observed in the Carina–Sagittarius Arm region (320° ≤ l ≤ 325°, |b| ≤ 1°) is an intrinsic structural feature of the spiral arm or a consequence of high interstellar reddening and ...
Corti M. A. +3 more
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Enhanced Resistive Switching Uniformity in Tantalum Oxide Memristor Devices via Copper Implantation
Advanced Electronic Materials, EarlyView.Metal oxide memristor devices typically suffer from uncontrolled forming processes and limited resistive switching uniformity due to the stochastic formation of an oxygen vacancy filament. Improved resistive switching uniformity in Ta2O5 memristor is developed by Cu implantation in the switching oxide.
Shaochuan Chen, Ilia Valov
wiley +1 more source
The Astronomical JournalWe present a spectroscopic study of young stellar clusters in the barred spiral galaxy NGC 1313. Integrated light spectra of 11 clusters, obtained using the GMOS-S instrument on the 8.1 m Gemini South telescope, are analyzed using a simple stellar ...
Jae-Rim Koo, Hyun-Jeong Kim, Beomdu Lim
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Fragmentation of young massive clusters in binary components: an application of Griddy Gibbs Sampler
Frontiers in Astronomy and Space SciencesThe study of the process of hierarchical fragmentation of molecular clouds within Young Massive Clusters required modeling the Initial Mass Function by considering both binary and single-star components.
Abisa Sinha Adhikary, Ankita Das
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Advanced Energy Materials, EarlyView.An alcohol‐adduct‐mediated strategy is employed to stabilize tin isopropoxide for the formation of a homogeneous double electron transport layer (ETL) incorporating SnO2 nanoparticles (NPs). This double‐ETL exhibits improved optical and charge‐transport properties due to reduced defect density and better energy level alignment, resulting in high ...
You‐Hyun Seo +10 more
wiley +1 more source
Probing Hadronic γ-Ray and High-energy Neutrino Emission from Gaia DR2 Star Clusters
The Astrophysical JournalYoung and massive stellar clusters are a potential source of galactic cosmic rays due to at least two acceleration mechanisms. Collective stellar winds from massive stars form a wind-blown bubble with a termination shock at which particle acceleration to
Alison M. W. Mitchell +4 more
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Young Massive Clusters in the Galactic Center
, 2004 The three young clusters in the Galactic Center represent the closest examples of massive starbursts and they define the upper mass limit of the Galactic cluster mass functions. In this review, I describe the characteristics and content of the Arches, Quintuplet, and Central clusters. They each are more massive than any other cluster in the Galaxy, and
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Advanced Energy Materials, EarlyView.A coaxial, membrane‐integrated hollow fiber electrode assembly (HFEA) is developed for continuous marine carbon mineralization. By utilizing a sub‐millimeter inter‐electrode gap, the HFEA minimizes Ohmic losses, achieving 50% energy reduction and over 85% DIC removal.
Inhwan Park +5 more
wiley +1 more source