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Star Formation Studies
Two submm sources in the B1-b molecular cloud core. |
Image Credit: Hirano Naomi
Two submm sources in the B1-b molecular cloud core. (Left) Thermal dust emission at 1.1 mm observed with the SMA (white contours) on top of the mid-IR image taken with the Spitzer space telescope (color image). (Right) N2D+ emission line observed with the SMA and SMT. (Huang & Hirano 2013, ApJ, 766, 131)
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