AFGL 915 - the Red Rectangle
Grayscale image of the 11.22 micron image of AFGL 915 from November
1994, taken at UKIRT with
The emission at this wavelength includes contributions from the warm
dust continuum and the strong unidentified IR emission feature at 11.2 microns.
The inner part of the nebula is saturated in this display to better
show the faint extensions from the corners of the ``rectangle". See
Hora, Deutsch, Hoffmann, & Fazio 1996, AJ, 112, 2064, for more information.
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Last modified 1997 December 9