COST Action Our Astrochemical History CM1401

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F60461373%3A22340%2F15%3A43900355" target="_blank" >RIV/60461373:22340/15:43900355 - isvavai.cz</a>
Result on the web
<a href="http://prague2015astrohistory.vscht.cz/" target="_blank" >http://prague2015astrohistory.vscht.cz/</a>
DOI - Digital Object Identifier
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Result language
angličtina
Original language name
COST Action Our Astrochemical History CM1401
Original language description
A large variety of chemical compounds, from hydrides to complex organic species, is observed in star and planet forming regions. These complex species are also detected in present-day comets and meteorites, possibly as witnesses of the early stages of Solar System formation. An active chemistry proceeds in the harsh environments of pre-stellar cores and proto-planetary disks, where UV photons or X-rays irradiate cold diluted gases and ices, and radicals are copiously produced. The aim of this Action isto bring together laboratory and theoretical gas phase and surface chemistry as well as large facilities based experiments with the aim of rationalizing the molecular evolution. Specific markers, such as isotopic fractionation, ices composition, and abundance ratios of isomers, must be used and understood, in order to draw a coherent picture of our chemical origins. Succeeding former European initiatives that shaped the field of Astrochemistry, this Action focuses on the molecular evolut
Czech name
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Czech description
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Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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