Results 221 to 230 of about 105,573 (267)
Ab-initio dynamic study of mechanisms for dust-mediated molecular hydrogen formation in space. [PDF]
Commun ChemGuo Y, McKenzie DR.
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The 130 to 375 GHz Rotational Spectroscopy of <i>s</i>-<i>trans</i>-(<i>Z</i>)-1-Cyano-1,3-butadiene (C<sub>5</sub>H<sub>5</sub>N): Analysis of the Lowest-Energy Vibrationally Excited Dyad (ν<sub>19</sub> and ν<sub>27</sub>). [PDF]
J Phys Chem ADorman PM +4 more
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Abiotic origin of the citric acid cycle intermediates. [PDF]
Proc Natl Acad Sci U S AMcAnally M +6 more
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Laboratory Infrared Spectra and Band Strengths of Carbonyl Sulfide (OCS) in CH<sub>3</sub>OH- and CO-Rich Ice Mixtures for Analyzing Interstellar Ice Observations. [PDF]
ACS Earth Space ChemSlavicinska K +5 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
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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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1987
Although most of the mass of the Milky Way Galaxy is condensed into stars, interstellar space is not completely empty. It contains gas and dust, in the form both of individual clouds and of a diffuse medium. Interstellar space typically contains about one gas atom per cubic centimetre and 100 dust particles per cubic kilometre.
Markku Poutanen +4 more
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Although most of the mass of the Milky Way Galaxy is condensed into stars, interstellar space is not completely empty. It contains gas and dust, in the form both of individual clouds and of a diffuse medium. Interstellar space typically contains about one gas atom per cubic centimetre and 100 dust particles per cubic kilometre.
Markku Poutanen +4 more
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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.
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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.
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The Interstellar Medium and the Intergalactic Medium
Astrophysics and Space Science, 2001Here we present a summary of the first discussion session on the interstellar and intergalactic medium.
José Franco, Gerhard Hensler
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