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A CO Survey of Giant Molecular Clouds near Cassiopeia A and NGC 7538

  • Authors: H. Ungerechts, P. Umbanhowar, and P. Thaddeus

Ungerechts, Umbanhowar, & Thaddeus 2000 The Astrophysical Journal 537 221.

  • Provider: AAS Journals

Caption: Fig. 3.

Molecular clouds in the Perseus arm toward Cassiopeia and Cepheus: ﹩^{13}﹩CO emission integrated over the velocity range −65 to −25 km s−1; there is no emission below −65 km s−1 in the area of the ﹩^{13}﹩CO map. The lowest contour is at 1.0 K km s−1, and each contour is again 1.58 times higher than the previous. The peak intensity is 25 K km s−1.

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