Results 11 to 20 of about 2,262 (175)

Methanetetrol and the final frontier in ortho acids [PDF]

open access: yesNature Communications
The rapid dissociation of methanetetrol (C(OH)4) has been suggested as an impediment to its observation, despite the stability of its substituted derivative orthocarbonates (C(OR)4).
Joshua H. Marks   +10 more
doaj   +2 more sources

The interstellar chemistry of C<sub>3</sub>H and C<sub>3</sub>H<sub>2</sub> isomers. [PDF]

open access: yesMon Not R Astron Soc, 2017
We report the detection of linear and cyclic isomers of C3H and C3H2 towards various starless cores and review the corresponding chemical pathways involving neutral (C3Hx with x=1,2) and ionic (C3Hx+ with x = 1,2,3) isomers. We highlight the role of the branching ratio of electronic Dissociative Recombination (DR) reactions of C3H2+ and C3H3+ isomers ...
Loison JC   +8 more
europepmc   +8 more sources

Computational investigation of spin-resolved energy landscapes of FeC4H2+ and their astrochemical implications [PDF]

open access: yesFrontiers in Chemistry
The enduring enigma of iron depletion in the interstellar medium serves as a compelling impetus for an in-depth exploration of iron-bearing molecular species.
Shilpa Shajan   +2 more
doaj   +2 more sources

The simplest iminophosphane HPNH and its photoisomerization to aminophosphinidene H2NP [PDF]

open access: yesNature Communications
As a heavy analogue of dinitrogen, the diatomic phosphorus mononitride (PN) was the first detected phosphorus-containing compound in the interstellar medium.
Junjie Jiang   +5 more
doaj   +2 more sources

Hydrogen ejection from hydrocarbons: Characterization and relevance in soot formation and interstellar chemistry [PDF]

open access: yesProceedings of the National Academy of Sciences of the United States of America
Josie Hendrix   +2 more
exaly   +2 more sources

Gas-phase Chemistry in the Interstellar Medium: The Role of Laboratory Astrochemistry

open access: yesFrontiers in Astronomy and Space Sciences, 2022
“Who” and how? In this simple question the complexity of the interstellar chemistry is encapsulated. “Who” refers to what molecules are present in the interstellar medium (ISM) and “how” to the mechanisms that led to their formation.
Cristina Puzzarini
doaj   +1 more source

Molecular Precursors of the RNA-World in Space: New Nitriles in the G+0.693−0.027 Molecular Cloud

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Nitriles play a key role as molecular precursors in prebiotic experiments based on the RNA-world scenario for the origin of life. These chemical compounds could have been partially delivered to the young Earth from extraterrestrial objects, stressing the
Víctor M. Rivilla   +15 more
doaj   +1 more source

Dust evolution, a global view I. Nanoparticles, nascence, nitrogen and natural selection … joining the dots [PDF]

open access: yesRoyal Society Open Science, 2016
The role and importance of nanoparticles for interstellar chemistry and beyond is explored within the framework of The Heterogeneous dust Evolution Model for Interstellar Solids (THEMIS), focusing on their active surface chemistry, the effects of ...
A. P. Jones
doaj   +1 more source

Dust evolution, a global view: III. Core/mantle grains, organic nano-globules, comets and surface chemistry [PDF]

open access: yesRoyal Society Open Science, 2016
Within the framework of The Heterogeneous dust Evolution Model for Interstellar Solids (THEMIS), this work explores the surface processes and chemistry relating to core/mantle interstellar and cometary grain structures and their influence on the nature ...
A. P. Jones
doaj   +1 more source

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