The IIM Stabilized with a Cubic Spline Model for the Source Function

Details The IIM Stabilized with a Cubic Spline Model for the Source Function The IIM Stabilized with a Cubic Spline Model for the Source Function

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..268c&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Statistics

Computation

Hii Regions, Infrared: Stars, Open Clusters And Associations: General, Stars: Early-Type

Scientific paper

The Integral Implicit Method (IIM) (Simonneau & Crivellari 1988)
solves the RT problems in stellar atmospheres model computations. A
cubic spline model assures the continuity of the source function and
that of the first and second derivatives at each discrete optical depth.

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