圖片來源: 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)
|