DePoy, D.L., Stephens, A., Martini, P., Harper, D.A., Lowenstein, R.F., Marks, R., Gatley, I., Fowler, A., and Sharp, N. to appear in "New Views of the Magellanic Clouds", IAU Symposium 190, July 1998
We have obtained infrared images of a 10' by 40' region from 30 Dor south to N159. There are JHK images taken from the CTIO 1.5m telescope and L (3.5 micron) taken from the South Pole Infrared Explorer 0.6m telescope. All the images reach a limiting sensitivity > 13 mag. The images allow us to identify many objects with infrared excesses, which are plausibly high mass pre-main sequence objects, and all Carbon stars and supergiants. The distribution of these sources may trace the star formation history of the 30 Dor complex.
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