Astrochemistry of Dust, Ice and Gas | Buch | 978-1-78262-128-7 | sack.de

Buch, Englisch, 400 Seiten, Format (B × H): 155 mm x 246 mm, Gewicht: 1089 g

Astrochemistry of Dust, Ice and Gas

Faraday Discussion 168
Erscheinungsjahr 2014
ISBN: 978-1-78262-128-7
Verlag: RSC Publishing

Faraday Discussion 168

Buch, Englisch, 400 Seiten, Format (B × H): 155 mm x 246 mm, Gewicht: 1089 g

ISBN: 978-1-78262-128-7
Verlag: RSC Publishing


Faraday Discussions covers a variety of topics in rapidly developing areas of the physical sciences, with a focus on physical chemistry and its interfaces with other scientific disciplines. The journal publishes the papers presented and a record of the questions, discussion and debate that took place at the corresponding Faraday Discussions meeting and provides an important record of current international knowledge and opinions in the relevant field. Each Faraday Discussion covers a topic in a rapidly developing area of chemistry and will be of interest to academic and industrial chemists across all areas of the chemical sciences.

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Weitere Infos & Material


- Astrochemistry of dust, ice and gas: introduction and overview

- The chemistry of planet-forming regions is not interstellar

- Exploring the origins of carbon in terrestrial worlds

- Complex molecule formation around massive young stellar objects

- Chemical complexity in the Horsehead, photodissociation region

- General discussion

- Efficient diffusive mechanisms of O atoms at very low temperatures on surfaces of astrophysical interest

- Single and double addition of oxygen atoms to propyne on surfaces at low temperatures

- Reaction kinetics and isotope effect of water formation by the surface reaction of solid H2O2 with H atoms at low temperatures

- Diffusion of atomic oxygen relevant to water formation in amorphous interstellar ices

- Polycyclic aromatic hydrocarbons– catalysts for molecular hydrogen formation

- Electron induced chemistry: a new frontier in astrochemistry

- Low-energy electron-induced chemistry of condensed methanol: implications for the interstellar synthesis of prebiotic molecules

- Stability of carbonaceous dust analogues and glycine under UV irradiation and electron bombardment

- General discussion

- The cycling of carbon into and out of dust

- The formation of ice mantles on interstellar grains revisited – the effect of exothermicity

- Characterizing the chemical pathways for water formation – a deep search for hydrogen peroxide

- The formation of glycine and other complex organic molecules in exploding ice mantles

- Complex organic molecules along the accretion flow in isolated and externally irradiated protoplanetary disks

- General discussion

- Cold condensation of dust in the ISM

- THz and mid-IR spectroscopy of interstellar ice analogs: methyl and carboxylic acid groups

- Infrared and reflectron time-of-flight mass spectroscopic study on the synthesis of glycolaldehyde in methanol (CH3OH) and methanol–carbon monoxide (CH3OH–CO) ices exposed to ionization radiation

- Application of a diffusion–desorption rate equation model in astrochemistry

- Wavelength resolved UV photodesorption and photochemistry of CO2 ice

- Free-electron laser induced processes in thin molecular ice

- General discussion

- Concluding remarks: astrochemistry of dust, ice and gas


Faraday Discussions documents a long-established series of Faraday Discussion meetings which provide a unique international forum for the exchange of views and newly acquired results in developing areas of physical chemistry, biophysical chemistry and chemical physics. The papers presented are published in the Faraday Discussion volume together with a record of the discussion contributions made at the meeting. Faraday Discussions therefore provide an important record of current international knowledge and views in the field concerned. The latest (2012) impact factor of Faraday Discussions is 3.82.



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