Radiative transfer in molecular lines

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/10261/2665

Full metadata record

DC Field	Value	Language
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	-
Appears in Collections:	Digital Csic

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