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Long Baseline Observations of the HD 100546 Protoplanetary Disk with ALMA

  • Authors: Sebastián Pérez, Simon Casassus, Antonio Hales, Sebastián Marino, Anthony Cheetham, Alice Zurlo, Lucas Cieza, Ruobing Dong, Felipe Alarcón, Pablo Benítez-Llambay, Ed Fomalont, and Henning Avenhaus

2020 The Astrophysical Journal Letters 889 L24.

  • Provider: AAS Journals

Caption: Figure 4.

Same as Figure 3, but for 13CO emission. The white dashed contours show the corresponding 12CO emission at 10 and 16 times the 12CO maps rms, while the gray solid contour shows 13CO at 3 times the rms level. The 7 km s−1 channel most clearly shows that 13CO do not exhibit the same obvious wiggle as in 12CO.

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