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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 17.

The 13CO integrated intensity of the Taurus molecular cloud overlaid with the integrated prediction of feedback position from ME1 along velocity channels in red. The arcs in yellow indicate the position of previously identified bubbles in Li et al. (2015). The star symbols demonstrate the locations of the Class III YSOs from Kraus et al. (2017).An interactive version of this figure is available.

An interactive version of this figure is available in the online journal.

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