Interstellar nitrogen chemistry
La nouvelle fenêtre spectroscopique dans le sub-millimétrique, ouverte par l’avènement del’observatoire spatial Herschel, a permis la détection d’espèces azotées simples, les hydruresd’azote NH, NH2 et NH3, dans les enveloppes froides de proto-étoiles. Ces enveloppes sontconstituées de gaz dense et froid caractéristique des conditions physico-chimiques
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Cryogenic Bottom-up Formation of the Benzene Cation from Acetylene in Helium Nanodroplets. [PDF]
Foitzik F +5 more
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Interstellar Stereoisomerism. [PDF]
Rivilla VM, Sanz-Novo M, San Andrés D.
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Atom Addition Formation of Thionylimide (HNSO) on Interstellar Dust Grains: Chemical Routes Requiring Oxygen and Nitrogen Atom Surface Diffusion. [PDF]
Del Valle JC +6 more
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Formation of Monocyclic and Polycyclic Hydrocarbons from Sequential Toluene Reactions in Coulomb Crystals. [PDF]
Kocheril GS +3 more
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Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
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Abiotic formation of nitrile precursors to amino acids and nucleobases in interstellar ice analogues. [PDF]
Wang J +8 more
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Wavelength-dependent photofragmentation of pyrazine. [PDF]
Payra SS, Thakkar P, Lenka Y, Aravind G.
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Laboratory Investigation of Simultaneous Ultraviolet Photoprocessing and Temperature-Programmed Desorption of Interstellar Ice Analogs. [PDF]
Sarver CC, Walker CE, Widicus Weaver SL.
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Low-energy glycine formation and spectral masking in star-forming regions. [PDF]
Mates-Torres E, Rimola A.
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