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Application of Convolutional Neural Networks to Identify Stellar Feedback Bubbles in CO Emission

  • Authors: Duo Xu, Stella S.R. Offner, Robert Gutermuth, and Colin Van Oort

2020 The Astrophysical Journal 890 64.

  • Provider: AAS Journals

Caption: Figure 6.

Results of the eight models applied to Rank A bubble TMB12. First row, first column panel: integrated intensity of 13CO overlaid with a yellow ring indicating the position and thickness of the bubble. Star symbols show the location of the Class III YSOs from Kraus et al. (2017). The remaining panels show the predicted intensity integrated along the velocity axis for the eight CNN models.

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