Results 61 to 70 of about 2,211 (208)
New calculations have been applied to the pyrolysis of pyrrole under shock‐tube conditions and to the radical‐radical reaction between allyl and •CN at low temperature and pressure, using the same mechanistic scheme for both. ABSTRACT The pyrolysis of pyrrole has previously been studied in shock‐tube experiments and in jet‐stirred reactors. The results
Barry K. Carpenter
wiley +1 more source
RF plasma production and electron processing of interstellar carbonaceous dust analogs.
Carbonaceous dust in the diffuse interstellar (IS) medium is largely made of some sort of amorphous hydrogenated carbon (a-C:H), whose structure has been explained by two alternative models: small aromatic islands linked by aliphatic chains [1] or large polyaromatic structures with small aliphatic substituents at the edges [2].
Peláez, Ramón J. +7 more
+7 more sources
Observation of Diffuse Galactic Light Near the Galactic Center with ONC-T on Board Hayabusa2
Diffuse Galactic light (DGL) is starlight scattered by interstellar dust. In visible wavelengths, earlier studies observed DGL toward regions of low optical depth in high Galactic latitude, and show marginal consistency with a theoretical model assuming ...
Kei Sano +23 more
doaj +1 more source
The spectral features and detectability of small, cyclic silicon carbide clusters
Rovibrational spectral data for several tetra-atomic silicon carbide clusters (TASCCs) are computed in this work using a CCSD(T)-F12b/cc-pCVTZ-F12 quartic force field.
Christopher M. Sehring +3 more
doaj +1 more source
The Dynamics of Reading Genre Fiction: Researching and Teaching Interpretive Practices
Conceptual model positioning genre fiction as a site for studying how narrative form organizes reader interpretation, identifying four dynamics—iterability, narrative interest, serialization, and spectacle—to guide empirical research on reading processes.
Robert Jean LeBlanc, Amy Stornaiuolo
wiley +1 more source
Analysis of the 3.2–3.3 μm Interstellar Absorption Feature on Three Milky Way Sightlines
We report new analyses of spectra of the 3.2–3.3 μ m absorption feature observed in the diffuse interstellar medium toward three Milky Way sources: 2MASS J 17470898 − 2829561 (2M1747) and the Quintuplet Cluster, both located in the Galactic center, and ...
L. S. Bernstein, T. R. Geballe
doaj +1 more source
Abstract Xenon (Xe) is a heavy noble gas with intriguing chemical properties, such as having several stable isotopes and the ability to form compounds under extreme conditions. Despite the predictions based on cosmochemical models that suggest xenon should be relatively abundant in planetary reservoirs, empirical data indicate a significant depletion ...
Avinash Kumar Both +2 more
wiley +1 more source
Effects of cosmic rays on hydrocarbon interstellar dust
International audienceHydrogenated amorphous carbons, an important component of the interstellar carbonaceous dust, possess infrared spectral signatures (at 3.4, 6.9 and 7.3 µm) that are ubiquitous in the diffuse interstellar medium of galaxies, but not ...
Godard, Marie +10 more
core +1 more source
The Flattest Infrared Extinction Curve in Four Isolated Dense Molecular Cloud Cores
The extinction curve of interstellar dust in the dense molecular cloud cores is crucial for understanding dust properties, particularly size distribution and composition.
Jun Li +5 more
doaj +1 more source
State of the Early Career Profession in Space Physics and Aeronomy: Climatological Survey Results
Abstract The American Geophysical Union (AGU) Space Physics & Aeronomy (SPA) section comprises scientists who study the Sun, solar wind, and planetary magnetospheres, ionospheres, and thermospheric/mesospheric systems along with their interconnections.
R. C. Allen +11 more
wiley +1 more source

