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http://arxiv.org/pdf/1309.7792...
Part of book or chapter of book
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Oskar Bordeaux
Part of book or chapter of book . 2013
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Part of book or chapter of book . 2013
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Part of book or chapter of book . 2013 . 2012
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Astrochemistry: Synthesis and modelling

Wakelam, V.; Cuppen, H.M.; Herbst, E.; Smith, I.W.M.; Cockell, C.S.; Leach, S.;

Astrochemistry: Synthesis and modelling

Abstract

2013, IX, 349 p. 79 illus., 55 in color; International audience; We discuss models that astrochemists have developed to study the chemical composition of the interstellar medium. These models aim at computing the evolution of the chemical composition of a mixture of gas and dust under astrophysical conditions. These conditions, as well as the geometry and the physical dynamics, have to be adapted to the objects being studied because different classes of objects have very different characteristics (temperatures, densities, UV radiation fields, geometry, history etc); e.g., proto-planetary disks do not have the same characteristics as proto-stellar envelopes. Chemical models are being improved continually thanks to comparisons with observations but also thanks to laboratory and theoretical work in which the individual processes are studied.

Countries
France, France, Netherlands
Subjects by Vocabulary

Microsoft Academic Graph classification: Physics Computational physics Interstellar medium Chemical composition Astrochemistry Astrophysics Work (thermodynamics) Chemical models

arXiv: Astrophysics::Galaxy Astrophysics

Keywords

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]

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  • citations
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    7
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    Average
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visibility
citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
views
OpenAIRE UsageCountsViews provided by UsageCounts
7
Average
Average
Average
11
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Funded by
EC| KISMOL
Project
KISMOL
Kinetics in Soft Molecular Layers - from interstellar ices to polymorph control
  • Funder: European Commission (EC)
  • Project Code: 259510
  • Funding stream: FP7 | SP2 | ERC
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