Nuclear structure of NGC 3379

Details Nuclear structure of NGC 3379 Nuclear structure of NGC 3379

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...140..174b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 140, no. 1, Nov. 1984, p. 174-176.

Astronomy and Astrophysics

Astrophysics

7

Convolution Integrals, Galactic Nuclei, Galactic Structure, Astronomical Photography, High Resolution, Point Sources, Spectral Resolution

Scientific paper

A deconvolution procedure was carried out on a high resolution photographic profile of NGC 3379 in an attempt to discern the presence of a point-like source for an observed light cusp in previous scans. Gaussian PSF components in radially symmetric images of the object were expanded in a finite series of gaussian functions. A linear system of equation was extracted from the series approximation and solved with a regularization technique. The calculation failed to confirm the presence of a point source brighter than 21B mag. Further studies with the Space Telescope are recommended.

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