Results 121 to 130 of about 4,557 (177)
Secondary Ion-Ice Chemistry in UV-Irradiated Oxygen Ice: New Astrochemical Models Including Bulk Ionic Species. [PDF]
ACS Earth Space ChemDarnell K +8 more
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Cryogenic Bottom-up Formation of the Benzene Cation from Acetylene in Helium Nanodroplets. [PDF]
J Am Chem SocFoitzik F +5 more
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Chemistry in Extreme Environments: The Mystery of Molecular Complexity in Space. [PDF]
ACS Cent SciPuzzarini C, Alessandrini S.
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Modeling the radiolysis in H<sub>2</sub>O : HCOOH ice: connecting laboratory experiments with astronomical measurements. [PDF]
RSC AdvFargnoli CMF, Moraes L, Pilling S.
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Computational investigation of spin-resolved energy landscapes of FeC<sub>4</sub>H<sub>2</sub> <sup>+</sup> and their astrochemical implications. [PDF]
Front ChemShajan S, Thirumoorthy K.
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The Formation of Glycolamide on Interstellar Ices. [PDF]
ACS Cent SciViti S.
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2021
Except in particular situations, the behaviour of ordinary gases is adiabatic. In fact, due to the low values of the viscosity coefficients and thermal conductivity there is no thermal contact with the surrounding medium and the dissipation of energy by viscosity is negligible.
Shantanu Basu, Pranav Sharma
+4 more sources
Except in particular situations, the behaviour of ordinary gases is adiabatic. In fact, due to the low values of the viscosity coefficients and thermal conductivity there is no thermal contact with the surrounding medium and the dissipation of energy by viscosity is negligible.
Shantanu Basu, Pranav Sharma
+4 more sources
Oxygen in the Interstellar Medium
Reviews in Mineralogy and Geochemistry, 2008The oxygen that is observed in the Solar System today is a remnant of the interstellar oxygen that was in the dense molecular cloud that collapsed to form the Solar System. While the chemical evolution of the Galaxy has progressed since then, processes in the interstellar medium (ISM) that involve oxygen are relevant to the origins of oxygen in the ...
Kemper, Ciska +3 more
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Space Science Reviews, 2005
Infrared spectroscopy and photometry with ISO covering most of the emission range of the interstellar medium has led to important progress in the understanding of the physics and chemistry of the gas, the nature and evolution of the dust grains and also the coupling between the gas and the grains.
Abergel, A. +4 more
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Infrared spectroscopy and photometry with ISO covering most of the emission range of the interstellar medium has led to important progress in the understanding of the physics and chemistry of the gas, the nature and evolution of the dust grains and also the coupling between the gas and the grains.
Abergel, A. +4 more
openaire +2 more sources