Radiative transfer in molecular lines

dc.creator	Asensio Ramos, Andrés
dc.creator	Trujillo Bueno, J.
dc.creator	Cernicharo, José
dc.date	2008-01-09T16:20:02Z
dc.date	2008-01-09T16:20:02Z
dc.date	2001-02-15
dc.date.accessioned	2017-01-31T00:59:40Z
dc.date.available	2017-01-31T00:59:40Z
dc.identifier	arXiv:astro-ph/0102270v1
dc.identifier	http://hdl.handle.net/10261/2665
dc.identifier.uri	http://dspace.mediu.edu.my:8181/xmlui/handle/10261/2665
dc.description	The highly convergent iterative methods developed by Trujillo Bueno and Fabiani Bendicho (1995) for radiative transfer (RT) applications are generalized to spherical symmetry with velocity fields. These RT methods are based on Jacobi, Gauss-Seidel (GS), and SOR iteration and they form the basis of a new NLTE multilevel transfer code for atomic and molecular lines. The benchmark tests carried out so far are presented and discussed. The main aim is to develop a number of powerful RT tools for the theoretical interpretation of molecular spectra.
dc.description	Peer reviewed
dc.format	437229 bytes
dc.format	application/pdf
dc.language	eng
dc.relation	Preprint
dc.rights	openAccess
dc.subject	Methods: numerical
dc.subject	Radiative transfer
dc.subject	Stars:atmospheres
dc.subject	Missions: FIRST
dc.title	Radiative transfer in molecular lines
dc.type	Pre-print

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