Results 111 to 120 of about 476,181 (204)
Rotational equilibrium of C2 in diffuse interstellar clouds
Context. Recent spectroscopic measurements have revealed absorption from higher rotational levels in C2 than previous observations. These improvements are accompanied by the availability of updated radiative and collisional data. Aims. We revisit the density and radiation field intensity diagnostics provided by the observations of many rotational ...
J. Le Bourlot +4 more
openaire +2 more sources
First identified in 1964, inverse Raman scattering (IRS) is a nonlinear stimulated phenomenon that induces Raman-scattered absorptions where Raman emissions would be expected.
Frédéric Zagury
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Infrared spectra of hydrocarbon dust absorption bands toward the bright hypergiant Cygnus OB2-12 are compared to published spectra of the Quintuplet Cluster, a sightline to the Galactic center. The Cyg OB2-12 data include a new ground-based 2.86−3.70 μ m
Yvonne J. Pendleton +16 more
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Gas-phase Oxygenation and Sulfurization Processes of Fullerene Cations
Atomic oxygen and sulfur are known to efficiently react with fullerenes and may thus form a long list of oxygenated and sulfurated fullerene species in the interstellar medium (ISM).
Nian Zhao +6 more
doaj +1 more source
Método sem malha hp-clouds na análise de placas Reissner-Mindlin / [PDF]
Dissertação (Mestrado) - Universidade Federal de Santa Catarina, Centro Tecnológico.O conteúdo deste trabalho trata da aplicação do método sem malha hp-Clouds ou simplesmente método de nuvens (C. A. Duarte e J. T.
Garcia, Oscar Alfredo
core
Putting the Diffuse Interstellar Bands on the Map – Literally!
In a quest to further our understanding of the diffuse interstellar medium (ISM) as well as the unidentified carriers of the diffuse interstellar bands (DIBs), we are mapping DIBs across the sky using hundreds of hot stars as background torches ...
van Loon, J. Th.
core +1 more source
Extinction Distributions in Nearby Star-resolved Galaxies. II. M33
Extinction maps are essential for tracing interstellar dust and enabling accurate stellar population studies in galaxies. Here, a high-resolution extinction distribution of the nearby Triangulum galaxy (M33), is constructed by fitting multiband color ...
Yuxi Wang +4 more
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The tendency of some diffuse interstellar band (DIB) carriers to concentrate in the outer UV-illuminated layers of molecular clouds (MCs), the so-called skin effect, makes their spatial distribution a powerful probe of their physical nature. We leveraged
Zhao H., Li L.
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$C_{3}$ EXCITATION PROFILES IN DIFFUSE INTERSTELLAR CLOUDS
Department of Astronomy, University of California, Berkeley, CA 94720.Author Institution: Department of Chemistry, University of California; Division of Geological and Planetary Sciences 150-21, California Institute of Technology; Department of Chemistry,
Blake, Geoffrey A. +2 more
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The Gas-phase Nitridation Processes of Fullerene Cations in the Interstellar Medium
The chemical evolution of fullerene molecules is an important and interesting topic in astrochemistry. In this work, the coevolution processes occurring in fullerene cations ([C _60 ] ^+ and [C _58/56 ] ^+ ) in response to ultraviolet radiation and N ...
Yanan Ge +3 more
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