Results 131 to 140 of about 4,398 (186)

Non-equilibrium preparation of (<i>E</i>)-phosphinimine (HPNH, X¹A') - a precursor to prebiotic phosphorylating agents. [PDF]

Chem Sci
Wang J, Sun BJ, Bergantini A, Wang Z, McAnally M, Marks JH, Chang AHH, Eckhardt AK, Kaiser RI.   +8 more
europepmc   +1 more source

The IMAP Observatory Overview. [PDF]

Space Sci Rev
Hegarty KP, Kubota S, Cully M, McComas DJ, Christian ER, Schwadron NA, Gkioulidou M, Bushman S, Collura C, Dauberman M, Drabenstadt C, Driesman A, Dubill A, Duffy B, Coleman E, Eng D, Ercol CJ, Gerger A, Hall R, Hahn J, Haque M, Hefter S, Jeong D, Jones D, Kelman J, Krupiarz C, Kujawa F, Lippe C, Matlin D, Monaco C, Myers D, Rivera Sepulveda E, Rodriguez D, Roufberg L, Scherrer J, Schwinger M, Shin A, Siddique F, Smith E, Smith R, Tapley M, Vernon S, Vigil C, Weidner S.   +43 more
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Increased and varied radiation during the Sun's encounters with cold clouds in the last 10 million years. [PDF]

Sci Rep
Opher M, Giacalone J, Loeb A, Economo EP, Cummings A, Middleton J, Zucker C, Miller JA, Nica A, Hatzaki M.   +9 more
europepmc   +1 more source

Formation of Monocyclic and Polycyclic Hydrocarbons from Sequential Toluene Reactions in Coulomb Crystals. [PDF]

J Phys Chem A
Kocheril GS, Zagorec-Marks C, Allison SH, Lewandowski HJ.   +3 more
europepmc   +1 more source

Interstellar Stereoisomerism. [PDF]

ACS Earth Space Chem
Rivilla VM, Sanz-Novo M, San Andrés D.
europepmc   +1 more source

Nonequilibrium Synthesis of Glycolamide (NH₂COCH₂OH), a Precursor to Amino Acids, on Interstellar Nanoparticles. [PDF]

ACS Cent Sci
Bergantini A, Wang J, Antonov I, Batrakova EA, Tuchin SO, Kaiser RI.   +5 more
europepmc   +1 more source

Rotational Characterization of Four-Ring Polycyclic Aromatic Hydrocarbons: Toward the Detection of Fluoranthene and Cyanofluoranthene in Space. [PDF]

J Phys Chem Lett
Villar-Castro D, Cabezas C, Steber AL, Morán JR, de la Fuente S, Hussain FS, Pérez D, Lesarri A, Cernicharo J, Pérez C, Peña I.   +10 more
europepmc   +1 more source

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The Interstellar Medium

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
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The Cool Interstellar Medium

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., Verstraete, L., Joblin, C., Laureijs, R., A. Miville-Deschênes, M.   +4 more
openaire   +2 more sources

Oxygen in the Interstellar Medium

Reviews in Mineralogy and Geochemistry, 2008
The 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, Jensen, Adam G., Markwick-Kemper, F., Snow, Theodore P.   +3 more
openaire   +1 more source