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More π, please: What drives the formation of unsaturated molecules in the interstellar medium? [PDF]
Chem SciLondoño-Restrepo J +4 more
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Interstellar Ices: A Factory of the Origin-of-Life Molecules. [PDF]
ACS Cent SciPuzzarini C, Alessandrini S.
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Protein language models enable accurate viral host range prediction. [PDF]
Sci RepBeltrán JF +3 more
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Laboratory infrared spectra and fragmentation chemistry of sulfur allotropes. [PDF]
Nat CommunFerrari P +4 more
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Escape From X Chromosome Inactivation as a Driver of Plasmacytoid DC Heterogeneity in Health and Disease. [PDF]
Immunol RevBarrat FJ, Guéry JC.
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A visualizable and widely applicable steric repulsion descriptor for guiding experimental chemistry. [PDF]
Chem SciJust GH +5 more
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Chemistry of Diffuse Molecular Clouds toward Sagittarius B2
Chemistry of Diffuse Molecular Clouds toward Sagittarius B2openaire
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Diffuse Atomic and Molecular Clouds
Annual Review of Astronomy and Astrophysics, 2006Diffuse interstellar clouds have long been thought to be relatively devoid of molecules, because of their low densities and high radiation fields. However, in the past ten years or so, a plethora of polyatomic molecules have been observed in diffuse clouds, via their rotational, vibrational, and electronic transitions.
Benjamin Mccall, Theodore P Snow
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