The Effect of an Inert Solid Reservoir on Molecular Abundances in Dense Interstellar Clouds
The question, what is the role of freeze-out of chemical species in determining the molecular abundances in the interstellar gas is a matter of debate.
Kalvāns Juris, Shmeld Ivar
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A study of X-ray point sources in Heiles Clouds 1 and 2
Star formation takes place in the coldest parts of molecular clouds, beginning in the densest, collapsing regions of filaments. As pre-main sequence stars are luminous X-ray emitters, X-ray point sources can serve as effective tracers of YSOs.
Nóra Varga +2 more
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Cosmic-Ray Induced Diffusion in Interstellar Ices
Cosmic rays are able to heat interstellar dust grains. This may enhance molecule mobility in icy mantles that have accumulated on the grains in dark cloud cores.
Kalvāns Juris
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Molekul antar Bintang dan Struktur Galaksi
Ringkasan. Tulisan ini merupakan tinjauan ulang penemuan molekul di dalam ruang antarbintang, kemungkinan pembentukannya dan kaitannya dengan struktur Galaktika. Abstract.
Bambang Hidajat
doaj
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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The Transition from Atomic to Molecular Hydrogen in Interstellar Clouds: 21 cm Signature of the Evolution of Cold Atomic Hydrogen in Dense Clouds [PDF]
P. F. Goldsmith, Di Li, Marko Krčo
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Modelling the dust emission from dense interstellar clouds: disentangling the effects of radiative transfer and dust properties [PDF]
N. Ysard +23 more
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Anomalous Neutral Hydrogen Column Densities in Local Interstellar Medium Clouds
Analysis of high-resolution spectra of the hydrogen and deuterium Ly α lines provides measurements of interstellar neutral hydrogen column densities N (H i ) to 113 stars within 50 pc of the Sun. Plots of N (H i ) versus distance through the LIC, G, Mic,
Jeffrey L. Linsky, Seth Redfield
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Why HOC[TSUP]+[/TSUP] Is Detectable in Interstellar Clouds: The Rate of the Reaction between HOC[TSUP]+[/TSUP] and H[TINF]2[/TINF] [PDF]
Eric Herbst, David E. Woon
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Search for Interstellar Water in the Translucent Molecular Cloud toward HD 154368 [PDF]
Marco Spaans +4 more
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