dc.creatorOCTAVIO CARDONA NUÑEZ
dc.creatorMONICA MIGUEL MARTINEZ ARROYO
dc.creatorMARIA DE LOS ANGELES LOPEZ CASTILLO
dc.date2010-03-01
dc.date.accessioned2023-07-25T16:23:42Z
dc.date.available2023-07-25T16:23:42Z
dc.identifierhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1456
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7806652
dc.descriptionA new approximate partition function is derived as a function of temperature and total number density of particles in the given system, and three adjustable parameters. The derivation assumes that we can simulate the calculations of the partition function for hydrogen by means of averages of the energies and sums of the statistical weights.We present the procedure and mathematical process to obtain an approximate analytic function and its derivatives that depend on those parameters. The comparisons with other calculations reported in the literature show good agreement. The free parameters of this function are calculated and given in a table for all the ions of the first 20 atomic species.
dc.formatapplication/pdf
dc.languageeng
dc.publisherThe Astrophysical Journal
dc.relationcitation:Cardona, O. et al., (2010). Atomic partition function for stellar atmospheres and plasma diagnostics, The Astrophysical Journal. Vol. 711(1):239-245
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0
dc.subjectinfo:eu-repo/classification/Inspec/Atomic processes
dc.subjectinfo:eu-repo/classification/Inspec/Equation of state
dc.subjectinfo:eu-repo/classification/Inspec/Plasmas
dc.subjectinfo:eu-repo/classification/Inspec/Stars: atmospheres
dc.subjectinfo:eu-repo/classification/cti/1
dc.subjectinfo:eu-repo/classification/cti/21
dc.subjectinfo:eu-repo/classification/cti/21
dc.titleAtomic partition function for stellar atmospheres and plasma diagnostics
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/acceptedVersion
dc.audiencestudents
dc.audienceresearchers
dc.audiencegeneralPublic


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