Kinetic database for astrochemistry
EAS Publications Series, ISSN: 1633-4760, Vol: 58, Page: 287-290
2012
- 2Citations
- 61Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Conference Paper Description
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. KIDA was designed to group at the same place and with the same format all gas-phase chemical reactions useful for astrochemical simulations of the interstellar medium and planetary atmospheres. From KIDA, a subset of chemical reactions has been extracted for the cold and dense interstellar medium: kida.uva.2001. © The Author(s) 2013.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84874378137&origin=inward; http://dx.doi.org/10.1051/eas/1258047; http://www.eas-journal.org/10.1051/eas/1258047; http://www.eas-journal.org/10.1051/eas/1258047/pdf; https://dx.doi.org/10.1051/eas/1258047; https://www.eas-journal.org/articles/eas/abs/2012/06/eas1258047/eas1258047.html
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