Results 171 to 180 of about 41,542 (217)

Global Reaction Route Mapping of C₃H₂O: Isomerization Pathways, Dissociation Channels, and Bimolecular Reaction with a Water Molecule. [PDF]

Molecules
Zhang D, Kishimoto N.
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Evaluating Infrared Absorption Parameters for Low-Temperature Ices Using Reflection-Absorption Infrared Spectroscopy. [PDF]

ACS Earth Space Chem
Fulker JE, McCoustra M, Brown WA.
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Insights Into the Gas-Phase Structure and Internal Dynamics of Diphenylsilane: A Broadband Rotational Spectroscopy Study. [PDF]

Chemphyschem
Batra G, Schnell M.
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Addressing electronic and dynamical evolution of molecules and molecular clusters: DFTB simulations of energy relaxation in polycyclic aromatic hydrocarbons.

Phys Chem Chem Phys
Rapacioli M, Buey MY, Spiegelman F.
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Supernovae and interstellar gas dynamics

Symposium - International Astronomical Union, 1967
The efficiency of the transfer of energy from supernovae into interstellar cloud motions is investigated. A lower limit of about 0·002 is obtained, but values near 0·01 are more likely. Taking all uncertainties in the theory and observations into account, the energy per supernova, in the form of relativistic particles or high-velocity matter, needed to
F. D. Kahn, L. Woltjer
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Whistlers in interstellar gas dynamics

AIP Conference Proceedings, 2002
Based on equation of electromagnetic induction for the magnetic flux density driven by Hall and Ohmic components of electric field generated by flows of thermal electrons an analytic model of helicoidal magneto-electron waves, whistlers, is developed.
Jongmann Yang, D. V. Podgainy, Sergey Bastrukov   +2 more
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Interstellar Gas Dynamics

Publications of the Astronomical Society of Australia, 1968
It is a well established observational result that young stars exhibit differences in chemical composition. The differences are comparatively large. For example, some stars have metal abundances as high as 3/2 solar-value while others have abundances as low as 1/2 solar-value.
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