The nucleus of M32 at 0.2 arcsec resolution

Details The nucleus of M32 at 0.2 arcsec resolution The nucleus of M32 at 0.2 arcsec resolution

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aj....104...83l&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 104, no. 1, July 1992, p. 83-91.

Astronomy and Astrophysics

Astronomy

22

Brightness Distribution, Charge Coupled Devices, Galactic Structure, High Resolution, Seeing (Astronomy), Angular Resolution, Black Holes (Astronomy), Galactic Nuclei, Point Spread Functions, Telescopes

Scientific paper

High-resolution multicolor CCD images of the nucleus of M32 obtained with the image-stabilization high-resolution camera on the Canada-France-Hawaii Telescope are analyzed. Results confirm the central flattening of the surface brightness profile of M32, as indicated by the lower-resolution photometry of Tonry (1987) and Michard and Nieto (1991). The central slope of the deconvolved surface brightness profile of M32 is consistent with a range of power-law index gamma between values of -0.8 and 0.

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