Results 221 to 230 of about 5,023,389 (339)
Advanced Materials Interfaces, EarlyView.This study introduces an approach for creating liquid‐like slippery surfaces (LLS) on various substrates. An epoxy‐silicon (EpSi) coating is applied, plasma‐activated, and immersed in an organosilane solution, forming siloxane chains. The resulting LLS exhibits ultra‐low ice adhesion, high transparency, self‐cleaning, and anti‐staining properties ...
Amirhossein Jalali Kandeloos +6 more
wiley +1 more source
Galactic Chemical Evolution Models Favor an Extended Type Ia Supernova Delay-time Distribution
The Astrophysical JournalType Ia supernovae (SNe Ia) produce most of the Fe-peak elements in the Universe and therefore are a crucial ingredient in galactic chemical evolution models.
Liam O. Dubay +2 more
doaj +1 more source
The Distribution of OB Stars in the Northern Milky Way [PDF]
, 1968 M. E. Sim
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Advanced Materials Interfaces, EarlyView.Unique nanopillar metasurfaces are fabricated for the purpose of sensitive detection to refractive index changes in the presence of gold nanoparticles. The addition of these nanoparticles to the surface of the silicon nanopillars is facilitated via a novel antibiotic‐mediated linker system to promote localized surface plasmon effects resulting from Mie
Jacob Waitkus +4 more
wiley +1 more source
Advanced Materials Interfaces, EarlyView.Herein, polymer nanogels with a reporting interface for albumin are synthesized through reversible addition–fragmentation chain transfer (RAFT) precipitation polymerization of di(ethylene glycol) methyl ether methacrylate and N,N’‐methylenebis(acrylamide) using a poly(2‐methacryloyloxyethyl phosphorylcholine) macro‐RAFT agent, followed by dansyl ...
Yukiya Kitayama +2 more
wiley +1 more source
A Catalog of Distance Determinations for 5 Million Stars in LAMOST DR10
The Astronomical JournalUsing the distance estimation method outlined in J. L. Carlin et al., a Bayesian approach specifically tailored for LAMOST data, we estimated distances for 7,450,303 spectra from 5,394,174 unique stars in the LAMOST DR10 low-resolution data set.
Chengqun Yang +5 more
doaj +1 more source
The distribution of young stars, clusters and cepheids in the Milky Way and M33 - a comparison [PDF]
, 1979 R. M. Humphreys
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Advanced Materials Technologies, EarlyView.A QR code, printed through a commercial printer on a thin plastic foil, pre‐coated with a nanocavity is proposed as an anti‐counterfeiting label. Nanocavity imparts distinctive optical properties in terms of light reflection and transmission. A thin layer of polymer‐dispersed liquid crystals (PDLC) is used to camouflage the QR code, that become ...
Giuseppe Nicoletta +6 more
wiley +1 more source
Radial Wave in the Galactic Disk: New Clues to Discriminate Different Perturbations
The Astrophysical JournalDecoding the key dynamical processes that shape the Galactic disk structure is crucial for reconstructing the Milky Way’s evolution history. The second Gaia data release unveils a novel wave pattern in the L _Z −〈 V _R 〉 space, but its formation ...
Chengye Cao +3 more
doaj +1 more source
1.2.3 Scattering in the Earth’S Atmosphere: Calculations for Milky Way and Zodiacal Light as Extended Sources [PDF]
, 1976 H. J. Staude
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