Results 111 to 120 of about 2,067,931 (248)
The Distribution of Interstellar Molecules in Dust Clouds as Derived from Laboratory Experiments [PDF]
, 1973 H. D. Breuer
openalex +1 more source
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
doaj +1 more source
Laboratory Studies of the Spectra of Interstellar Molecules [PDF]
, 1971 G. Herzberg
openalex +1 more source
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
doaj +1 more source
Molecule Formation in Cool, Dense Interstellar Clouds [PDF]
, 1980 W. D. Watson
openalex +1 more source
Sticking coefficients for atoms and molecules at the surfaces of interstellar dust grains [PDF]
, 1985 M. A. Leitch-Devlin, D. A. Williams
openalex +1 more source
Infrared intensities and molar refraction of amorphous dimethyl carbonate - comparisons to four interstellar molecules. [PDF]
Phys Chem Chem Phys, 2019 Hudson RL, Coleman FM.
europepmc +1 more source
On the Initial Excitation Temperature of Interstellar H_{2}CO Molecules
, 1970 Takeshi Oka
openalex +1 more source
Long Chain Carbon Molecules in the Interstellar Medium [PDF]
, 1980 L. W. Avery
openalex +1 more source