An astrophysics data program investigation of spatial structure of supernova remnants

Details An astrophysics data program investigation of spatial structure of supernova remnants An astrophysics data program investigation of spatial structure of supernova remnants

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993sao..reptq....h&link_type=abstract

Final Report, 1 Aug. 1989 - 31 Jul. 1991 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Fourier Transformation, Software Tools, Supernova Remnants, X Ray Imagery, Brightness, High Resolution, Power Spectra

Scientific paper

The final report on astrophysics data program investigation of spatial structure of supernova remnants for the period 1 Aug. 1989 to 31 Jul. 1991 is presented. The goal of the project was the study of the spatial structure of supernova remnants (SNR's) as observed in the x-ray band. A number of software tools were developed for the analysis: (1) a program to fit various geometric models to high resolution x-ray data, and (2) programs for Fourier Transform analysis of clumping in SNR's. These programs were applied to high resolution imager (HRI) data on the young galactic SNR's Tycho and Kepler with some success.

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