Results 171 to 180 of about 219,513 (216)

Aryl radical addition-dehydrocyclization drives rapid polycyclic aromatic hydrocarbon growth. [PDF]

Nat Commun
Goettl SJ, Sun BJ, Turner AM, Drissi M, Garcia GA, Nahon L, Kadam KP, Chang AHH, Kaiser RI.   +8 more
europepmc   +1 more source

Swift Heavy Ion-Induced Chemistry of CH₃CN Ices at 10 and 80 K. [PDF]

ACS Earth Space Chem
de Barros ALF, da Costa CAP, Murhej Y, Sreeja R, Doreste DV, da Silveira EF, Bouduch P, Rothard H, Michielan M, Ascenzi D, Domaracka A.   +10 more
europepmc   +1 more source

Pyrrole without Life: Reaction of Aminomethylene with the Propargyl Radical. [PDF]

J Phys Chem Lett
McClish R, Schleier D, Kamer J, Kasper T, Hemberger P, Bodi A, Bouwman J.   +6 more
europepmc   +1 more source

Simulations of multi-phase gas in and around galaxies. [PDF]

Living Rev Comput Astrophys
Gronke M, E Schneider E.
europepmc   +1 more source

Isomer-specific excitation of formic acid in collisions with helium atoms.

Phys Chem Chem Phys
Sogomonyan K, Veselinova-Marinova A, Lique F, Loreau J.   +3 more
europepmc   +1 more source

The acceleration of interstellar clouds

, 1954
openaire   +1 more source

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Interstellar Molecules and Dense Clouds

Science, 1971
Current knowledge of the interstellar medium is discussed on the basis of recent published studies. The subjects considered include optical identification of interstellar molecules, radio molecular lines, interstellar clouds, isotopic abundances, formation and disappearance of interstellar molecules, and interstellar probing techniques.
C H Townes
exaly   +3 more sources

FRACTAL ASPECTS OF INTERSTELLAR CLOUDS

Fractals, 1993
Interstellar matter consisting of gas and dust shows structures which appear to have self-similar projected shapes, similar to the properties of terrestrial clouds. Moreover, the completely different physics in these interstellar clouds reveals several additional self-similar/fractal aspects which are investigated by extensive astronomical ...
Zimmermann, Thomas, Stutzki, Jürgen
openaire   +2 more sources

The chemical composition of interstellar molecular clouds

Origins of Life, 1984
The published version is located at http://www.springerlink.com/content/w327411847532321/
Irvine, William M., HJALMARSON, A
openaire   +3 more sources

Interstellar Dust Clouds

Nature, 1971
THE failure, thus far, to detect gaseous emission lines from circumstellar dust clouds1–3 and from Bok globules2 raises the possibility that such clouds consist solely of dust grains. The possibility has previously been largely discounted on the grounds that relative diffusion of the grains and gas is slow and inefficient requiring time scales which ...
openaire   +2 more sources