Three-dimensional deconvolution of X-ray emission from AR Lac

Details Three-dimensional deconvolution of X-ray emission from AR Lac Three-dimensional deconvolution of X-ray emission from AR Lac

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.259..453s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 259, no. 3, p. 453-456.

Astronomy and Astrophysics

Astronomy

16

Eclipsing Binary Stars, Imaging Techniques, Stellar Coronas, X Ray Astronomy, X Ray Stars, Image Processing, Iteration, Light Curve

Scientific paper

A simple iterative method for the three-dimensional deconvolution of the X-ray light curves of eclipsing binaries is presented. The procedure allows the spatial distribution of the X-ray emission to be obtained without a priori assumptions about the localization, number or size of the emitting structures. The method is used for mapping the corona of the eclipsing binary AR Lac.

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