Results 91 to 100 of about 3,228 (211)

The UMIST database for astrochemistry 1995

open access: yes, 1996
We report the release of a new version of the UMIST database for astrochemistry. The database contains the rate coefficients of 3864 gas-phase reactions important in interstellar and circumstellar chemistry and involves 395 species and 12 elements.
Willacy, K.   +5 more
core   +1 more source

Editorial: Refractory Astrochemistry

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Ryan C. Fortenberry   +2 more
doaj   +1 more source

Astrochemistry in an Ion Storage Ring

open access: yes, 2012
Storage ring studies of low energy electron collisions with molecular ions have been carried out for dissociative recombination (DR) of fluorine-bearing molecules. Here we report on work aiming to improve the understanding of astrochemistry involving HF,
Orlov, D. A.   +19 more
core   +1 more source

Metal-ion mediated photolytic regulation of diphenylalanine stability: Implications for prebiotic chemical evolution

open access: yesiScience
Summary: Early Earth’s UV-rich environment, together with abundant transition metals, likely shaped the stability of biomolecules. We investigated how cations influence the UV (254 nm) stability of diphenylalanine (FF).
Wei Tang   +8 more
doaj   +1 more source

Astrochemistry: an unfinished symphony

open access: yes, 2009
Alex Dalgarno has introduced many of the themes that define current research in astrochemistry. Variations on these themes will continue to be played out well into the future. Clear and unambiguous tests of theories of formation of interstellar molecules
Black, John H,
core   +1 more source

Infrared Spectroscopic and Physical Properties of Methanol Ices—Reconciling the Conflicting Published Band Strengths of an Important Interstellar Solid

open access: yesThe Astrophysical Journal
Infrared spectroscopic observations have established the presence of solid methanol (CH _3 OH) in the interstellar medium and in solar system ices, but the abundance of frozen CH _3 OH cannot be deduced without accurate band strengths, optical constants,
Reggie L. Hudson   +2 more
doaj   +1 more source

Astrochemistry and Observations [PDF]

open access: yes, 1997
8 pages, 6 figures in text, From Fourth Cologne-Bonn-Zermatt-Symposium, The Dense Interstellar Matter in ...
openaire   +2 more sources

Experimental and Computational Laboratory Astrochemistry – A Personal View

open access: yes, 2021
The application of surface science methodologies to problems in solid state and surface laboratory astrochemistry has seen rapid growth and considerable success over the last two decades.
McCoustra, Martin R. S.; id_orcid
core  

Carbon Dioxide Ices—A Sexagennial Update of Infrared Intensities, Band Shapes, and the Formation and Destruction of Crystalline CO2

open access: yesThe Astrophysical Journal
The infrared (IR) band strengths most often used to quantify laboratory and astronomical spectra of CO _2 ices are now 60 yr old, from a time of slide rules and vacuum-tube technology.
Reggie L. Hudson   +2 more
doaj   +1 more source

The UMIST database for astrochemistry 1999

open access: yes, 2000
We report a new version of the UMIST database for astrochemistry. The previous (1995) version has been updated and its format has been revised. The database contains the rate coefficients, temperature ranges and - where available - the temperature ...
Le Teuff, Y.H.   +6 more
core   +1 more source

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