Results 211 to 220 of about 54,240 (242)
Studying Pure CH<sub>4</sub> and the Interaction of CH<sub>4</sub> and H<sub>2</sub>O in Interstellar Ice Analogues with On-Resonance Infrared Irradiation. [PDF]
Schrauwen JGM +3 more
europepmc +1 more source
Flux equipartition in astrophysical plasma turbulence. [PDF]
Marino R, Xie JH.
europepmc +1 more source
JWST Observations of Segregated <sup>12</sup>CO<sub>2</sub> and <sup>13</sup>CO<sub>2</sub> Ices in Protostellar Envelopes. [PDF]
Brunken NGC +15 more
europepmc +1 more source
Hot Sulfur on the Rocks: The Reaction of Electronically Excited Sulfur Atoms with Water in an Ice-Surface Model. [PDF]
Di Genova G +5 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
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
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
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 ...
openaire +2 more sources
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 ...
openaire +2 more sources
Interstellar Molecules and Dense Clouds
Science, 1971Current 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.
D M, Rank, C H, Townes, W J, Welch
openaire +2 more sources
FRACTAL ASPECTS OF INTERSTELLAR CLOUDS
Fractals, 1993Interstellar 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

