Publicação: The formation of CN and CN+ by direct radiative association
dc.contributor.author | Singh, P. D. | |
dc.contributor.author | Andreazza, C. M. | |
dc.contributor.institution | Universidade de São Paulo (USP) | |
dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
dc.date.accessioned | 2014-02-26T17:10:18Z | |
dc.date.accessioned | 2014-05-20T14:15:58Z | |
dc.date.available | 2014-02-26T17:10:18Z | |
dc.date.available | 2014-05-20T14:15:58Z | |
dc.date.issued | 2000-07-01 | |
dc.description.abstract | Rate coefficients for direct radiative association of carbon and nitrogen atoms to form CN, and of carbon ions and nitrogen atoms to form CN+ ions, are calculated for temperatures in the range of 300 to 14,700 K. For the CN molecule, the rate coefficients can be represented by the standard expression, k(CN)(T) = 7.87 x 10(-19)(T/300)(0.056) exp (-96.0/T) cm(3) s(-1) for temperatures between 300 and 2700 K and k(CN)(T) = 1.37 x 10(-18)(T/300)-0.128 exp (-520.1/T) cm(-3) s(-1) at T > 2700 K. For the CN+ ion, the corresponding expression is k(CN+)(T) = 1.08 x 10(-18)(T/300)(0.071) exp (-57.5/T) cm(-3) s(-1) for the temperature range studied. Calculated rate coefficients k(CN) are about 2 orders of magnitude lower than the canonical value used in the modeling of the chemistry of various astrophysical environments. | en |
dc.description.affiliation | Univ São Paulo, Inst Astron & Geofis, BR-04301904 São Paulo, Brazil | |
dc.description.affiliation | Univ Estadual Paulista, Inst Geociencias & Ciências Exatas, DEMAC, BR-13500230 Rio Claro, SP, Brazil | |
dc.description.affiliationUnesp | Univ Estadual Paulista, Inst Geociencias & Ciências Exatas, DEMAC, BR-13500230 Rio Claro, SP, Brazil | |
dc.format.extent | 261-263 | |
dc.identifier | http://dx.doi.org/10.1086/309023 | |
dc.identifier.citation | Astrophysical Journal. Bristol: Iop Publishing Ltd, v. 537, n. 1, p. 261-263, 2000. | |
dc.identifier.doi | 10.1086/309023 | |
dc.identifier.issn | 0004-637X | |
dc.identifier.lattes | 6915586041935129 | |
dc.identifier.uri | http://hdl.handle.net/11449/24787 | |
dc.identifier.wos | WOS:000088371000023 | |
dc.language.iso | eng | |
dc.publisher | Iop Publishing Ltd | |
dc.relation.ispartof | Astrophysical Journal | |
dc.relation.ispartofjcr | 5.551 | |
dc.rights.accessRights | Acesso restrito | |
dc.source | Web of Science | |
dc.subject | atomic processes | pt |
dc.subject | ISM : molecules | pt |
dc.subject | molecular processes | pt |
dc.title | The formation of CN and CN+ by direct radiative association | en |
dc.type | Artigo | |
dcterms.license | http://iopscience.iop.org/page/copyright | |
dcterms.rightsHolder | Iop Publishing Ltd | |
dspace.entity.type | Publication | |
unesp.author.lattes | 6915586041935129[2] | |
unesp.author.orcid | 0000-0002-4948-9471[2] | |
unesp.campus | Universidade Estadual Paulista (UNESP), Instituto de Geociências e Ciências Exatas, Rio Claro | pt |
unesp.department | Estatística, Matemática Aplicada e Computação - IGCE | pt |
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