Molecular clouds and star formation toward the Galactic plane within 216.25° ≤ l ≤ 218.75° and −0.75° ≤ b ≤ 1.25°

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Fig. 16

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Convolved BGPS 1.1 dust continuum emission (white contours) overlaid on the ¹³CO (1–0) integrated intensity map. The ¹³CO (1–0) map has been integrated over the velocity range between 22 and 29 km s^-1. The contour for the BGPS 1.1 dust continuum emission corresponds to the threshold of flux densities, 0.09 Jy beam^-1.

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