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D. R. Ciardi, J. P. Williams, C. M. Telesco, R. S. Fisher, C. Packham, J. T. Radomski (University of Florida)
Obtained with the University of Florida mid-infrared imager OSCIR on the Gemini-North telescope, 10--20 \micron\ photometry of the Class 0 protostars associated with the L 1448N binary, L1448N(A) and L1448N(B), is presented. The binary components are separated by approximately 7\arcsec, and should be spatially resolved from each other by OSCIR on Gemini (FWHM resolution ~0\farcs 5 at \lambda ~ 20 \micron). Only L1448N(A) has been detected, which is, itself, unresolved. Photometry for L1448N(A) and upper limits for L1448N(B) are presented.