Results 121 to 130 of about 30,505 (211)
Radiative association in dense, H2-containing interstellar clouds
The Astrophysical Journal, 1976 A method for estimating the order of magnitude of rate coefficients of radiative association reactions involving polyatomic species is outlined. Calculations are undertaken on reactions of possible importance in dense interstellar clouds. Several of the calculated rate coefficients are utilized in a study of the gas phase syntheses of H/sub 2/CNH ...
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The Astrophysical JournalWe present some of the first infrared spectral maps acquired by SPHEREx. These maps, which to our knowledge are the largest of their type ever compiled in the near-infrared, reveal multiple strong lines due to interstellar ices and polycyclic aromatic ...
Joseph L. Hora +34 more
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The Magnetic Keys to Massive Star Formation: The Western η Carinae Giant Molecular Cloud
The Astrophysical JournalWe present SOFIA/HAWC+ continuum polarization data on the magnetic fields ( B fields) threading 17 pc-scale massive molecular clumps at the western end of the η Carinae giant molecular cloud (Region 9 of the Galactic Census of High- and Medium-mass ...
Peter J. Barnes +3 more
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Extinction Distributions in Nearby Star-resolved Galaxies. II. M33
The Astronomical JournalExtinction maps are essential for tracing interstellar dust and enabling accurate stellar population studies in galaxies. Here, a high-resolution extinction distribution of the nearby Triangulum galaxy (M33), is constructed by fitting multiband color ...
Yuxi Wang +4 more
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The Astrophysical JournalUsing high-resolution UV data obtained from the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope, we focus on eight sight lines along the Sun’s historical trajectory to reconstruct the morphology of our most recent interstellar ...
Hunter Vannier +5 more
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Dust emission and extinction in the Orion OMC-3 cloud
Astronomy & AstrophysicsContext. Dust is an important tracer of the structure of interstellar clouds, as well as a central factor in the thermal balance and chemistry of the clouds.
Juvela Mika, Ysard Nathalie
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The Astrophysical JournalSulfur-bearing molecules are key constituents of the interstellar medium (ISM). Particularly, hydrogen sulfide (H _2 S) and cyano (CN) radicals are key precursors of prebiotic molecules in the ISM.
María Antiñolo +8 more
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Photochemistry of interstellar molecules [PDF]
The photochemistry of two diatomic and eight polyatomic molecules is discussed quantitatively. For an interstellar molecule, the lifetime against photodecomposition depends upon the absorption cross section, the quantum yield or probability of ...
Stief, L. J.
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Hydrogen Chloride in Dense Interstellar Clouds
The Astrophysical Journal, 1974 A. Dalgarno +3 more
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Molecule Formation in Dense Interstellar Clouds
Molecule Formation in Dense Interstellar Clouds資料番号 ...
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