Results 91 to 100 of about 35,391 (195)
The ALCHEMI Atlas: Principal Component Analysis Reveals Starburst Evolution in NGC 253
The Astrophysical Journal Supplement SeriesMolecular lines are powerful diagnostics of the physical and chemical properties of the interstellar medium (ISM). These ISM properties, which affect future star formation, are expected to differ in starburst galaxies from those of more quiescent ...
Nanase Harada +26 more
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5 cm OH Masers in Northern Star Formation Regions
The Astronomical JournalWe present a 6.0 GHz excited-state OH maser survey toward 155 northern star formation regions utilizing the Shanghai Tianma Radio Telescope. In total, we detect 44 6.0 GHz OH masers, 8 of which are new detections (one at 6016 MHz, two at 6030 MHz, and ...
Hai-Hua Qiao +6 more
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Infrared intensities and molar refraction of amorphous dimethyl carbonate - comparisons to four interstellar molecules. [PDF]
Phys Chem Chem Phys, 2019 Hudson RL, Coleman FM.
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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 Synchrotron-based Far-infrared Spectrum of Propargylamine
The Astrophysical Journal Supplement SeriesPropargylamine (HC≡C–CH _2 –NH _2 ), with a triple bond and an amine group, is a nitrogen-bearing organic molecule of astrochemical interest due to its potential role as a precursor to aminoacetonitrile and other complex organic molecules in the ...
Tianhao Hu +4 more
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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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Indirect observation of unobservable interstellar molecules [PDF]
It is suggested that the abundances of neutral non-polar interstellar molecules unobservable by radio astronomy can be systematically determined by radio observation of the protonated ions.
Green, S. +3 more
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Chemistry in Extreme Environments: The Mystery of Molecular Complexity in Space. [PDF]
ACS Cent SciPuzzarini C, Alessandrini S.
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Abiotic formation of nitrile precursors to amino acids and nucleobases in interstellar ice analogues. [PDF]
Chem SciWang J +8 more
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