The Transition from Atomic to Molecular Hydrogen in Interstellar Clouds: 21 cm Signature of the Evolution of Cold Atomic Hydrogen in Dense Clouds [PDF]
, 2006 P. F. Goldsmith, Di Li, Marko Krčo
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A sequential acid-base (SAB) mechanism in the interstellar medium: The emergence of cis formic acid in dark molecular clouds [PDF]
, 2023 Juan García de la Concepción +7 more
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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]
, 1996 Eric Herbst, David E. Woon
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Interstellar clouds containing optically thick H2
The Astrophysical Journal, 1975 The theory of Black and Delgarno that the relative populations of the excited rotational levels of H2 can be understood in terms of cascading following absorption in the Lyman and Werner bands is employed to infer the gas densities and radiation fields within diffuse interstellar clouds containing H2 that is optically thin in those bands.
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Faraday tomography of LoTSS-DR2 data: III. Revealing the Local Bubble and the complex of local interstellar clouds in the high-latitude inner Galaxy [PDF]
A. Erceg +6 more
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The Formation of Large Hydrocarbons and Carbon Clusters in Dense Interstellar Clouds [PDF]
, 1997 Ryan P. A. Bettens, Eric Herbst
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The Passage of the Solar System through the Edge of the Local Bubble
The Astrophysical JournalThe Sun moves through the interstellar medium (ISM) at a velocity of ∼19 pc Myr ^−1 , making the conditions outside the solar system vary with time over millions of years.
Merav Opher +12 more
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Formation of carbonyl sulfide (OCS) via SH radicals in interstellar CO-rich ice under dense cloud conditions [PDF]
Julia C. Santos +2 more
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Cloud-cloud collisions in the interstellar medium
The Astrophysical Journal, 1980 Results are presented from time-dependent numerical simulations of cloud-cloud collisions in the interstellar medium. Special emphasis is placed on physically detailed models of cloud collisions. The numerical simulations include heating, cooling, thermal conductivity, self-gravity, and molecule formation; magnetic fields have been neglected.
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Extended Red Emission in High-Galactic Latitude Interstellar Clouds
, 2008 Adolf N. Witt +4 more
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