Results 111 to 120 of about 2,067,931 (248)
The Distribution of Interstellar Molecules in Dust Clouds as Derived from Laboratory Experiments [PDF]
H. D. Breuer
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On the Interpretation of Mid-infrared Absorption Lines of Gas-phase H2O as Observed by JWST/MIRI
Rovibrational 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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Laboratory Studies of the Spectra of Interstellar Molecules [PDF]
G. Herzberg
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The 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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Molecule Formation in Cool, Dense Interstellar Clouds [PDF]
W. D. Watson
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Sticking coefficients for atoms and molecules at the surfaces of interstellar dust grains [PDF]
M. A. Leitch-Devlin, D. A. Williams
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Infrared intensities and molar refraction of amorphous dimethyl carbonate - comparisons to four interstellar molecules. [PDF]
Hudson RL, Coleman FM.
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On the Initial Excitation Temperature of Interstellar H_{2}CO Molecules
Takeshi Oka
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Long Chain Carbon Molecules in the Interstellar Medium [PDF]
L. W. Avery
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