Deprojection of emission in axially symmetric transparent systems

Details Deprojection of emission in axially symmetric transparent systems Deprojection of emission in axially symmetric transparent systems

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...247..584l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 247, no. 2, July 1991, p. 584-589. Research supported by NSERC.

Astronomy and Astrophysics

Astrophysics

5

Brightness Distribution, Emissivity, Optical Thickness, Transparence, Algorithms, Iteration, Polynomials, Power Series

Scientific paper

The general problem of the deprojection of optically thin emission is examined for the case of axially symmetric emission. The iterative deconvolution technique introduced by Lucy (1974) is employed for the deprojection of two mathematical forms of emissivity. The method is stable and gives results that are physically probable, and the approach is of interest to the study of optically thin astronomical objects which are axially symmetric.

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