Results 91 to 100 of about 219,513 (216)
On the Genetic Relation Between Interstellar Clouds and Dust Clouds [PDF]
We propose that many of the denser dust clouds represent transient stages between the initiation of gravitational collapse of ordinary interstellar clouds by passage through a spiral galactic shock and the appearance of a stellar association. The interstellar gas is not processed at too rapid a rate (1) because the time spent between galactic shocks is
openaire +1 more source
Atomic and Molecular Gas in the Milky Way. I. Structure Decomposition
We present GDCluster, a fully automated algorithm for decomposing a spectral-line data cube of interstellar gas into coherent structures. Assuming a multi-Gaussian nature of observed spectra, GDCluster employs and augments the derivative spectroscopy ...
Xin Liu, Fujun Du
doaj +1 more source
Observations of molecules in diffuse interstellar clouds
We present results from observations of diffuse interstellar clouds, with discussion of their significance and including a historical survey to put the recent work into perspective.
Somerville, W.B., Crawford, Ian
core +1 more source
INTERSTELLAR CLOUDS BY SEARCHLIGHT
Interpretation of high-resolution observations of absorption by interstellar clouds of radiation from extragalactic sources should include the effect of the Earth's motion with respect to the source. High-resolution H I absorption profiles that are not heavily blended have been published for eight sources.
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The Chemistry of Cold, Dark Interstellar Clouds [PDF]
In recent years the nearby cold, dark clouds have been shown to possess a rich chemistry, with interesting differences with respect to warmer massive-star-forming regions and also among the cold clouds themselves. 39 molecular species are now known in these regions.
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Alfvén Waves in Dusty Interstellar Clouds
Dust particles in a plasma can be higWy charged, and can carry a proportion of the negative charge of the plasma. Even if this proportion is quite small, as in interstellar dusty clouds, it can have a large effect on hydromagnetic Alfvén waves ...
S. V. Vladimirov, N. F. Cramer
core +1 more source
Optical interstellar lines in dark clouds. [PDF]
<p>Published - <a href="/records/nj8w2-gpn05/files/1973ApJ___186__149C.pdf?download=1">1973ApJ___186__149C.pdf</a></p>
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Grains charges in interstellar clouds [PDF]
The charge of cosmic grains could play an important role in many astrophysical phenomena. It probably has an influence on the coagulation of grains and more generally on grain-grain collisions, and on interaction between charged particles and grains ...
Bel, N., Viala, Y. P., Lafon, J. P.
core
Ice chemistry in the dense, cold interstellar medium (ISM) is probably responsible for the formation of interstellar complex organic molecules (COMs). Recent laboratory experiments performed at T ∼ 4 K have shown that irradiation of CO:N _2 ice samples ...
Rafael Martín-Doménech +3 more
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Multi-phase interstellar clouds in the Vela SNR resolved with XMM-Newton
XMM-Newton spatial/spectral resolution and high effective area allow to deepen our knowledge about the shocks in Supernova Remnants and their interaction with the interstellar medium.
Maggio, A. +3 more
core +1 more source

