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Effects of aberration and advection on line formation

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dc.contributor.author Peraiah, A
dc.date.accessioned 2008-07-09T07:27:37Z
dc.date.available 2008-07-09T07:27:37Z
dc.date.issued 1991-10
dc.identifier.citation Astrophysical Journal, Part 1, Vol. 380, No.1, pp. 212 - 222 en
dc.identifier.issn 0004-637X
dc.identifier.uri http://hdl.handle.net/2248/2584
dc.description.abstract The effects of inclusion of the aberration and advection terms in the equation of the line transfer are studied. Spherical shells whose ratios of outer (B) to inner (A) radii (B/A) are 2, 5, and 10 and with line-center optical depths 500, 1300, and 1350 are considered. The velocities of expansion of the medium are set at 1000, 2000, 3000, 4000, and 5000 km/s. The line source functions and the corresponding profiles of lines are calculated. The individual and combined effects of the transverse and radial velocity gradients, and those of aberration and advection in plane-parallel and spherically symmetric geometries on the line source functions and the emerging line profiles are considered. It is found that large effects are generated in the radiation field when these physical mechanisms are taken into account in the transfer of the line radiation. The method for various velocity laws was tested and found to be stable. en
dc.format.extent 1154422 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher University of Chicago Press en
dc.relation.uri http://adsabs.harvard.edu/abs/1991ApJ...380..212P en
dc.subject Line shape en
dc.subject Line spectra en
dc.subject Radiative transfer en
dc.subject Stellar envelopes en
dc.subject Supernovae en
dc.subject Optical thickness en
dc.subject Radiation distribution en
dc.subject Spherical shells en
dc.title Effects of aberration and advection on line formation en
dc.type Article en


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