Sökning: WFRF:(Talbi N) > Hickson K. M. > The 2014 KIDA Netwo...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 03441naa a2200733 4500 | |
001 | oai:DiVA.org:su-117487 | |
003 | SwePub | |
008 | 150520s2015 | |||||||||||000 ||eng| | |
009 | oai:gup.ub.gu.se/226365 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1174872 URI |
024 | 7 | a https://doi.org/10.1088/0067-0049/217/2/202 DOI |
024 | 7 | a https://gup.ub.gu.se/publication/2263652 URI |
040 | a (SwePub)sud (SwePub)gu | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Wakelam, V.4 aut |
245 | 1 0 | a The 2014 KIDA Network for Interstellar Chemistry |
264 | c 2015-03-25 | |
264 | 1 | b American Astronomical Society,c 2015 |
338 | a print2 rdacarrier | |
500 | a AuthorCount:24; | |
520 | a Chemical models used to study the chemical composition of the gas and the ices in the interstellar medium are based on a network of chemical reactions and associated rate coefficients. These reactions and rate coefficients are partially compiled from data in the literature, when available. We present in this paper kida.uva.2014, a new updated version of the kida.uva public gas-phase network first released in 2012. In addition to a description of the many specific updates, we illustrate changes in the predicted abundances of molecules for cold dense cloud conditions as compared with the results of the previous version of our network, kida.uva.2011. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
653 | a astrochemistry | |
653 | a astronomical databases: miscellaneous | |
653 | a ISM: abundances | |
653 | a ISM: molecules | |
653 | a astrochemistry | |
653 | a astronomical databases: miscellaneous | |
653 | a ISM: abundances | |
653 | a ISM: molecules | |
700 | 1 | a Loison, J.-C4 aut |
700 | 1 | a Herbst, E.4 aut |
700 | 1 | a Pavone, B.4 aut |
700 | 1 | a Bergeat, A.4 aut |
700 | 1 | a Beroff, K.4 aut |
700 | 1 | a Chabot, M.4 aut |
700 | 1 | a Faure, A.4 aut |
700 | 1 | a Galli, D.4 aut |
700 | 1 | a Geppert, Wolf D.u Stockholms universitet,Fysikum4 aut0 (Swepub:su)wgeppert |
700 | 1 | a Gerlich, D.4 aut |
700 | 1 | a Gratier, P.4 aut |
700 | 1 | a Harada, N.4 aut |
700 | 1 | a Hickson, K. M.4 aut |
700 | 1 | a Honvault, P.4 aut |
700 | 1 | a Klippenstein, S. J.4 aut |
700 | 1 | a Le Picard, S. D.4 aut |
700 | 1 | a Nyman, Gunnar,d 1957u Gothenburg University,Göteborgs universitet,Institutionen för kemi och molekylärbiologi,Department of Chemistry and Molecular Biology4 aut0 (Swepub:gu)xnymgu |
700 | 1 | a Ruaud, M.4 aut |
700 | 1 | a Schlemmer, S.4 aut |
700 | 1 | a Sims, I. R.4 aut |
700 | 1 | a Talbi, D.4 aut |
700 | 1 | a Tennyson, J.4 aut |
700 | 1 | a Wester, R.4 aut |
710 | 2 | a Stockholms universitetb Fysikum4 org |
773 | 0 | t Astrophysical Journal Supplement Seriesd : American Astronomical Societyg 217:2q 217:2x 0067-0049x 1538-4365 |
856 | 4 | u https://arxiv.org/abs/1503.01594y arXiv:1503.01594 |
856 | 4 | u http://arxiv.org/pdf/1503.01594 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-117487 |
856 | 4 8 | u https://doi.org/10.1088/0067-0049/217/2/20 |
856 | 4 8 | u https://gup.ub.gu.se/publication/226365 |
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