Results 111 to 120 of about 35,251 (238)
On the Interpretation of Mid-infrared Absorption Lines of Gas-phase H2O as Observed by JWST/MIRI
The Astrophysical Journal Supplement SeriesRovibrational absorption lines of H _2 O in the 5–8 μ m wavelength range selectively probe gas against the mid-infrared continuum-emitting background of the inner regions of young stellar objects and active galactic nuclei and deliver important ...
Jialu Li +2 more
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The Distribution of Interstellar Molecules in Dust Clouds as Derived from Laboratory Experiments [PDF]
, 1973 H. D. Breuer
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Laboratory Studies of the Spectra of Interstellar Molecules [PDF]
, 1971 G. Herzberg
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The Astrophysical JournalThe most abundant interstellar molecule, molecular hydrogen (H _2 ), is practically invisible in cold molecular clouds. Astronomers typically use carbon monoxide (CO) to trace the bulk distribution and mass of H _2 in our galaxy and many others.
Michael P. Busch
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Boundary conditions for the paleoenvironment: Chemical and physical processes in the pre-solar nebula [PDF]
Detailed study of the first interstellar hydrocarbon ring, cyclopropenylidene (C3H2), is continuing. The singly deuterated isotope of this molecule, C3HD, was observed in several cold interstellar clouds.
Irvine, William M., Schloerb, F. Peter
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Molecule Formation in Cool, Dense Interstellar Clouds [PDF]
, 1980 W. D. Watson
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Composition, structure and chemistry of interstellar dust [PDF]
The observational constraints on the composition of the interstellar dust are analyzed. The dust in the diffuse interstellar medium consists of a mixture of stardust (amorphous silicates, amorphous carbon, polycyclic aromatic hydrocarbons, and graphite ...
Allamandola, Louis J. +1 more
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Sticking coefficients for atoms and molecules at the surfaces of interstellar dust grains [PDF]
, 1985 M. A. Leitch-Devlin, D. A. Williams
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