On The Youngest Members Of 30 Doradus As Seen With Spitzer/IRAC

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We have analysed several sets of images of 30 Doradus obtained with the IRAC and MIPS cameras of the Spitzer Space Telescope. Our goal is to identify the youngest protostars in 30 Dor, either by their very red colors or by their photometric variability. In order to do this, we are cross-correlating the Spitzer photometry with data obtained at other wavelengths, and with objects identified in previous papers as being possible protostar members of 30 Dor. We identify a set of new candidate protostars, provide new data for some of the previous candidates, and attempt to place the new candidates in context (e.g. where are they relative to other signposts of recent star-formation?). We hope to use these data to empirically determine the IR colors of high mass protostars and to place constraints on their photometric variability.

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