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Effects of redistribution with dipole scattering on line source functions

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dc.contributor.author Peraiah, A
dc.contributor.author Rangarajan, K. E
dc.date.accessioned 2009-01-23T15:08:59Z
dc.date.available 2009-01-23T15:08:59Z
dc.date.issued 1981-09
dc.identifier.citation Journal of Astrophysics and Astronomy, Vol. 2, No. 3, pp. 245 – 252 en
dc.identifier.issn 0250-6335
dc.identifier.uri http://hdl.handle.net/2248/4281
dc.description.abstract The partial frequency redistribution function for zero natural line width and dipole scattering is used to obtain a simultaneous solution of the statistical equilibrium and line transfer equations in the comoving frame of an expanding gas. A non-LTE, two-level atom in an expanding spherical medium is considered, and the population ratio of the two levels, N2/N1, is calculated. The upper level population (N2), initially set equal to zero, is found to be enhanced significantly from its initial value. Variation in the velocity gradient had little effect on the N2/N1 ratio when the geometrical thickness of the medium was three or ten times the stellar radius; when the thickness was increased to twenty times the central radius, however, the velocity gradients changed this ratio considerably in the region where log T is less than or equal to two, T being the total optical depth. en
dc.language.iso en en
dc.publisher Indian Academy of Sciences en
dc.relation.uri http://adsabs.harvard.edu/abs/1981JApA....2..245P en
dc.relation.uri http://www.springerlink.com/content/25n3h42r40831580/ en
dc.subject Atmospheric Scattering en
dc.subject Frequency Distribution en
dc.subject Radiative Transfer en
dc.subject Spectral Line Width en
dc.subject Stellar Atmospheres en
dc.subject Stellar Atmospheres en
dc.subject Equilibrium Equations en
dc.subject Statistical Analysis en
dc.subject Stellar Magnitude en
dc.title Effects of redistribution with dipole scattering on line source functions en
dc.type Article en


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