Results 61 to 70 of about 3,801,891 (296)

Dust Absorption toward Supernova Remnant W44

open access: yesThe Astronomical Journal
Supernova remnants (SNRs) can strongly affect the chemical composition of the interstellar dust. In this paper, we investigate to what degree the dust and ices are modified by observing four stars expected to be absorbed by a giant molecular cloud ...
Tian-Yu Tu   +3 more
doaj   +1 more source

Modeling of diffuse molecular gas applied to HD 102065 observations

open access: yes, 2008
Aims. We model a diffuse molecular cloud present along the line of sight to the star HD 102065. We compare our modeling with observations to test our understanding of physical conditions and chemistry in diffuse molecular clouds. Methods.
Nehmé, Cyrine   +9 more
core   +1 more source

Organic Materials of Tomorrow: Horizons of Artificial Intelligence

open access: yesAdvanced Materials, EarlyView.
This review examines machine learning techniques accelerating the discovery of organic semiconductors by linking molecular structure to properties. Key methods include graph neural networks, generative models, and active learning. Applications to organic photovoltaics demonstrate practical impact.
Harold Mena   +3 more
wiley   +1 more source

“Smelltronics”—From Gas to Smell Sensing

open access: yesAdvanced Materials, EarlyView.
The emerging field of smelltronics, encompassing sensing technologies for complex volatile organic compounds, holds significant potential for extracting valuable chemical information. It facilitates the noninvasive, real‐time monitoring of humans, food, and the environment.
Takeshi Ono   +7 more
wiley   +1 more source

Galactic Cosmic Ray Interaction with the Perseus Giant Molecular Cloud Using Geant4 Monte Carlo Simulation

open access: yesUniverse
Galactic cosmic rays (GCRs), composed of protons and atomic nuclei, are accelerated in sources such as supernova remnants and pulsar wind nebulae, reaching energies up to the PeV range.
Luan Torres, Luiz Augusto Stuani Pereira
doaj   +1 more source

Atomic and Molecular Data for Diffuse Cloud Chemistry [PDF]

open access: yesHighlights of Astronomy, 1989
ABSTRACTA brief overview of the procedure for modeling diffuse interstellar clouds is given, and specific needs for atomic and molecular data are pointed out.
openaire   +1 more source

Gamma-ray emission from molecular clouds with the Cherenkov Telescope Array and the cosmic ray spectrum in the Galaxy [PDF]

open access: yes, 2022
In this work we calculate the diffuse emission from molecular clouds (MCs) in the Galaxy at very high energy (from hundreds of GeV to hundreds of TeV).We present the results from the analysis of the simulated emission of these sources as it will be ...
Peron, Giada
core  

Large‐Scale Determination of Frontier Orbital Energies of Disordered Small‐Molecule Organic Semiconductors Using Exciplex Emission Spectra

open access: yesAdvanced Materials, EarlyView.
ABSTRACT Accurately knowing the frontier orbital energies of the structurally disordered small‐molecule organic semiconductors that are used in optoelectronic devices such as organic light‐emitting diodes is required to rationally improve their performance. Here, we show that these energies can be deduced with a large accuracy from the peak energies of
Christian B. McDonald   +7 more
wiley   +1 more source

Ambipolar Diffusion in Molecular Cloud Cores and the Gravomagneto Catastrophe [PDF]

open access: yesThe Astrophysical Journal, 2007
This paper re-examines the problem of ambipolar diffusion as a mechanism for the production and runaway evolution of centrally condensed molecular cloud cores, a process that has been termed the gravomagneto catastrophe. Our calculation applies in the geometric limit of a highly flattened core and allows for a semi-analytic treatment of the full ...
Adams, Fred C., Shu, Frank H.
openaire   +2 more sources

Detection of hydrogen fluoride absorption in diffuse molecular clouds with Herschel/HIFI: an ubiquitous tracer of molecular gas [PDF]

open access: yes, 2010
International audienceWe discuss the detection of absorption by interstellar hydrogen fluoride (HF) along the sight line to the submillimeter continuum sources W49N and W51.
R. Güsten   +160 more
core   +1 more source

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