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RII partial frequency redistribution function and its effects on the formation of lines in expanding spherical atmospheres

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dc.contributor.author Peraiah, A
dc.date.accessioned 2010-02-19T12:42:56Z
dc.date.available 2010-02-19T12:42:56Z
dc.date.issued 1979-11
dc.identifier.citation Kodaikanal Observatory Bulletins Series A, Vol. 2, No. 3, pp. 203 – 212 en
dc.identifier.issn 0374-3632
dc.identifier.uri http://hdl.handle.net/2248/5022
dc.description.abstract The redistribution in frequency in lines formed in atmospheres in which the matter is moving radially outwards with velocity gradients is studied in the rest frame of the star. We velocity gradients is studied in the rest frame of the star. We have considered the RII angle averaged function (see Hummer 1962) with radiation damping in the atom’s rest frame and assumed a non LTE two level atom. en
dc.language.iso en en
dc.publisher Indian Institute of Astrophysics en
dc.rights © Indian Institute of Astrophysics en
dc.subject RII Partial Frequency Redistribution Function en
dc.subject Radiative Transfer in Spherical Symmetry en
dc.subject Expanding Atmospheres en
dc.subject Line Formation:Stellar Atmospheres en
dc.subject Radiative Transfer en
dc.title RII partial frequency redistribution function and its effects on the formation of lines in expanding spherical atmospheres en
dc.type Article en


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