, 2007 Using a newly developed Spatial Heterodyne Spectrometer (SHS), we have obtained the first radial velocity resolved emission-line profiles of diffuse [OII] λ3726 and λ3729 doublet emission from the warm (104 K) ionized component of our Galaxy\u27s ...
Roesler, F. L. +4 more
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Interstellar Stereoisomerism. [PDF]
ACS Earth Space ChemRivilla VM, Sanz-Novo M, San Andrés D.
europepmc +1 more source
A cosmic-ray loaded nascent outflow driven by a massive star cluster. [PDF]
Nat CommunLemoine-Goumard M +8 more
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Search for Line Emission from Interstellar OH Radicals.
The Astronomical Journal, 1964 openaire +2 more sources
Constraining the magnetohydrodynamic turbulence around Geminga by observing the γ-ray halo beyond 100 TeV. [PDF]
Sci AdvTibet ASγ Collaboration.
europepmc +1 more source
Mid-infrared Spectroscopy of Protonated Benzonitrile, 2-Cyanonaphthalene, and 9-Cyanoanthracene for Astrochemical Consideration. [PDF]
ChemphyschemRasmussen AP +6 more
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Shock-induced nucleation of nanophase Fe-Ni alloy and its implications for interstellar iron reservoirs. [PDF]
Front ChemVelampatti Selvaraj P, Chandrasekaran V.
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[CII] Emission in a Self-Regulated Interstellar Medium
The [CII] 157.74 $\mu$m fine structure transition is one of the brightest and most well-studied emission lines in the far-infrared (FIR), produced in the interstellar medium (ISM) of galaxies.
Hu, Chia-Yu +3 more
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New Electronic Transition of Ovalene in Solid <i>para</i>-H<sub>2</sub>: The S<sub>1</sub>-S<sub>0</sub> Transition with Its Origin at 19 400 cm<sup>-1</sup>. [PDF]
J Phys Chem LettWeber I, Langner J, Witek HA, Lee YP.
europepmc +1 more source
Gamma-ray line emission from $^7$Li and $^7$Be production by cosmic-rays
, 2000 We calculate the total gamma-ray line emission at ~450 keV that accompanies 7-Li and 7-Be production by cosmic-ray interactions, including the delayed line emission at 0.478 MeV from 7-Be radioactive decay.
Vangioni-Flam, E. +3 more
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