NGC 7129

Physics

Scientific paper

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Scientific paper

We plan IRS observations of two mid-IR excess objects in the young cluster NGC 7129 in order to establish that we can identify disk gap objects solely on the basis of the combined IRAC and MIPS photometry. By establishing that the combined IRAC and MIPS SEDs are a reliable method for detecting disk gaps, we can examine how frequently gaps occur in our sample of 30 young stellar clusters, and assess whether giant planet formation commonly occurs in the first few million years.

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