Laboratory Investigation of Simultaneous Ultraviolet Photoprocessing and Temperature-Programmed Desorption of Interstellar Ice Analogs. [PDF]
ACS Earth Space ChemSarver CC, Walker CE, Widicus Weaver SL.
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Interstellar formation of 1,2-propanediol (CH<sub>3</sub>CH(OH)CH<sub>2</sub>OH) and 1,2-ethenediol (HOCHCHOH)-key precursors to sugars and sugar derivatives. [PDF]
Chem SciWang J, Zhang C, Eckhardt AK, Kaiser RI.
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The simplest iminophosphane HPNH and its photoisomerization to aminophosphinidene H<sub>2</sub>NP. [PDF]
Nat CommunJiang J +5 more
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Global heliospheric termination shock strength in the solar-interstellar interaction. [PDF]
Nat AstronZirnstein EJ +6 more
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Multiscale Perspectives on Solid-Phase Astrochemistry: Laboratory, Computation, and Open Questions. [PDF]
Space Sci RevDickers MD +3 more
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The Influence of Chemical Structure on the Electronic Structure of Propylene Oxide. [PDF]
Int J Mol SciMatalon DG, Nixon KL, Jones DB.
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Rotationally Resolved Predissociation Spectrum of the 1<sup>5</sup>Φ ← X<sup>5</sup>Δ Rovibronic Band of FeH. [PDF]
J Phys Chem LettJin S +4 more
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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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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.
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Interstellar medium simulations
Astronomische Nachrichten, 2012AbstractIn this review we critically assess numerical simulations of the interstellar medium (ISM), and argue that 3D high resolution calculations are the most promising method to determine the structure of the interstellar gas and follow its evolution well into the nonlinear regime. Based on a Riemann solver adaptive mesh refinement code, we present a
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