Results 11 to 20 of about 10,794 (262)

Astrochemistry of Sub-Millimeter Sources in Orion: Studying the Variations of Molecular Tracers with Changing Physical Conditions [PDF]

open access: bronze, 2003
Cornerstone molecules (CO, H_2CO, CH_3OH, HCN, HNC, CN, CS, SO) were observed toward seven sub-millimeter bright sources in the Orion molecular cloud in order to quantify the range of conditions for which individual molecular line tracers provide ...
A. M. S. Boonman   +81 more
core   +6 more sources

Astrochemistry: overview and challenges [PDF]

open access: yesProceedings of the International Astronomical Union, 2017
This paper provides a brief overview of the journey of molecules through the Cosmos, from local diffuse interstellar clouds and PDRs to distant galaxies, and from cold dark clouds to hot star-forming cores, protoplanetary disks, planetesimals and ...
van Dishoeck, Ewine F.
core   +8 more sources

Computational challenges in Astrochemistry [PDF]

open access: greenWIREs Computational Molecular Science, 2017
Cosmic evolution is the tale of progressive transition from simplicity to complexity. The newborn universe starts with the simplest atoms formed after the Big Bang and proceeds toward ‘astronomical complex organic molecules’ (astroCOMs). Understanding the chemical evolution of the universe is one of the main aims of Astrochemistry, with the starting ...
Małgorzata Biczysko   +2 more
openalex   +5 more sources

Chemical Reactions in Astrochemistry [PDF]

open access: bronzeSymposium - International Astronomical Union, 1992
This paper is devoted to chemistry in the gas phase dealing firstly with ion-molecule reactions at extremely low temperature. The experimental techniques that have been used in this field are shortly presented and the reactions that have been studied using the CRESU(S) method reviewed.
B. R. Rowe
openalex   +3 more sources

Kinetic database for astrochemistry [PDF]

open access: bronzeEAS Publications Series, 2012
KIDA (for KInetic Database for Astrochemistry) is a project initiated by different communities in order to 1) improve the interaction between astrochemists and physico-chemists and 2) simplify the work of modeling the chemistry of astrophysical environments.
Valentine Wakelam, Tae Team
openalex   +3 more sources

A statistical and machine learning approach to the study of astrochemistry. [PDF]

open access: greenFaraday discussions, 2023
In order to obtain a good understanding of astrochemistry, it is crucial to better understand the key parameters that govern grain-surface chemistry. For many chemical networks, these crucial parameters are the binding energies of the species.
Johannes Heyl, S. Viti, G. Vermariën
semanticscholar   +3 more sources

Concluding remarks: Faraday Discussion on astrochemistry at high resolution. [PDF]

open access: hybridFaraday discussions, 2023
Fifty years on from the first detailed chemical kinetic modelling of astronomical sources, I provide some introductory comments on the history of astrochemistry, summarise some personal views on the topics covered in this discussion meeting, and conclude
T. Millar
semanticscholar   +3 more sources

Molecular Data Needs in Astrochemistry [PDF]

open access: bronzeSymposium - International Astronomical Union, 2000
The development of astrochemistry is inextricably linked to the generation of fundamental data. In this report, we discuss data needs in terms of astrochemical models, gas-phase kinetics, molecular excitation, optical and UV spectroscopy, solid-state chemistry, and millimeter and submillimeter wave spectroscopy.
T. J. Millar   +5 more
openalex   +4 more sources

Astrochemistry During the Formation of Stars [PDF]

open access: yesAnnual Review of Astronomy and Astrophysics, 2020
Star-forming regions show a rich and varied chemistry, including the presence of complex organic molecules—in both the cold gas distributed on large scales and the hot regions close to young stars where protoplanetary disks arise.
J. Jørgensen, A. Belloche, R. Garrod
semanticscholar   +7 more sources

LIDA: The Leiden Ice Database for Astrochemistry [PDF]

open access: yesAstronomy & Astrophysics, 2022
High quality vibrational spectra of solid-phase molecules in ice mixtures and for temperatures of astrophysical relevance are needed to interpret infrared observations toward protostars and background stars.
W. Rocha   +5 more
semanticscholar   +5 more sources

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