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dc.contributor.authorAndreazza, C. M.-
dc.contributor.authorMarinho, E. P.-
dc.contributor.authorSingh, P. D.-
dc.date.accessioned2014-02-26T17:27:08Z-
dc.date.accessioned2014-05-20T14:16:07Z-
dc.date.accessioned2016-10-25T17:39:17Z-
dc.date.available2014-02-26T17:27:08Z-
dc.date.available2014-05-20T14:16:07Z-
dc.date.available2016-10-25T17:39:17Z-
dc.date.issued2006-11-11-
dc.identifierhttp://dx.doi.org/10.1111/j.1365-2966.2006.10964.x-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society. Malden: Wiley-blackwell, v. 372, n. 4, p. 1653-1656, 2006.-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/11449/24847-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/24847-
dc.description.abstractThe rate coefficients for the formation of carbon monophosphide (CP) and silicon monophosphide (SiP) by radiative association are estimated for temperatures ranging from 300 to 14 100 K. In this temperature range, the radiative association rate coefficients are found to vary from 1.14 x 10(-18) to 1.62 x 10(-18) cm(3) s(-1) and from 3.73 x 10(-20) to 7.03 x 10(-20) cm(3) s(-1) for CP and SiP, respectively. In both cases, rate coefficients increase slowly with the increase in temperature.en
dc.format.extent1653-1656-
dc.language.isoeng-
dc.publisherWiley-Blackwell-
dc.sourceWeb of Science-
dc.subjectatomic datapt
dc.subjectatomic processespt
dc.subjectcircumstellar matterpt
dc.subjectISM : moleculespt
dc.titleRadiative association of C and P, and Si and P atomsen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv Estadual Paulista, IGCE, DEMAC, BR-13500230 Rio Claro, SP, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, IGCE, DEMAC, BR-13500230 Rio Claro, SP, Brazil-
dc.identifier.doi10.1111/j.1365-2966.2006.10964.x-
dc.identifier.wosWOS:000241626100017-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society-
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