Results 171 to 180 of about 7,455 (223)

Coupling laboratory FTIR data with PROCODA kinetic modeling for the radiolysis of frozen formic acid using swift ions. [PDF]

RSC Adv
Moraes L, Fargnoli CM, Pilling S.
europepmc   +1 more source

Fundamental Role of N-O Bond-Containing Compounds in Prebiotic Synthesis. [PDF]

JACS Au
Sukhorukov AY.
europepmc   +1 more source

Abiotic origin of the citric acid cycle intermediates. [PDF]

Proc Natl Acad Sci U S A
McAnally M, Bocková J, Turner AM, Hara N, Mikhnova D, Meinert C, Kaiser RI.   +6 more
europepmc   +1 more source

Investigation of positron scattering from atomic fluorine and fluorine-containing molecules. [PDF]

RSC Adv
Yadav A, Antony B.
europepmc   +1 more source

Physicochemical Properties of α‑Pinene in Water Ice Analogs under Energetic Heavy-Ion Irradiation. [PDF]

ACS Earth Space Chem
de Barros ALF, Doreste DV, Ricca A, Murhej Y, da Silveira EF, Boduch P, Rothard H, Domaracka A.   +7 more
europepmc   +1 more source

High-resolution spectroscopy of [H,C,N]⁺: II. Ground state rotational spectrum of HCN⁺ (<i>X̃</i>²Π).

Phys Chem Chem Phys
Silva WGDP, Schmid PC, Gupta D, Thorwirth S, Sarka J, Asvany O, Schlemmer S.   +6 more
europepmc   +1 more source

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Complex Organic Interstellar Molecules

Annual Review of Astronomy and Astrophysics, 2009
Of the over 150 different molecular species detected in the interstellar and circumstellar media, approximately 50 contain 6 or more atoms. These molecules, labeled complex by astronomers if not by chemists, all contain the element carbon and so can be called organic. In the interstellar medium, complex molecules are detected in the denser sources only.
Eric Herbst, E F Van Dishoeck
exaly   +3 more sources

Interstellar molecules

Journal of Molecular Evolution, 1980
B E Turner
exaly   +2 more sources

Interstellar Molecules

Journal of Molecular Evolution, 1974
The study of interstellar molecules broadly includes two areas of interest. One area uses the unique ability of molecules to act as probes of the physical conditions in the cold, dense, visually opaque component of the interstellar medium. The physical properties of this and other components of the interstellar medium are summarized.
openaire   +3 more sources