Results 171 to 180 of about 207,817 (216)

Electron-Impact Resonances of Anthracene in the Presence of Methanol: Does the Solvent Identity Matter? [PDF]

J Phys Chem Lett
Lietard A, Verlet JRR.
europepmc   +1 more source

IR-Action Spectroscopy of the Astrochemically Relevant HCCS⁺ Cation. [PDF]

ACS Earth Space Chem
Michielan M, Steenbakkers K, Ascenzi D, Diprose JA, Polášek M, Brünken S, Romanzin C, Heazlewood BR, Puzzarini C, Richardson V.   +9 more
europepmc   +1 more source

Low-energy glycine formation and spectral masking in star-forming regions. [PDF]

Commun Chem
Mates-Torres E, Rimola A.
europepmc   +1 more source

The acceleration of interstellar clouds

, 1954
openaire   +1 more source

High-resolution spectroscopy of [H,C,N]⁺: II. Ground state rotational spectrum of HCN⁺ (<i>X̃</i>²Π).

Phys Chem Chem Phys
Silva WGDP, Schmid PC, Gupta D, Thorwirth S, Sarka J, Asvany O, Schlemmer S.   +6 more
europepmc   +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.
W J Welch
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
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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
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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 ...
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Interstellar Molecular Clouds

Science, 1986
The interstellar medium in our galaxy contains matter in a variety of states ranging from hot plasma to cold and dusty molecular gas. The molecular phase consists of giant clouds, which are the largest gravitationally bound objects in the galaxy, the primary reservoir of material for the ongoing birth of new stars, and the medium regulating the ...
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