Figure 3 from Application of Convolutional Neural Networks to Identify Stellar Feedback Bubbles in CO Emission

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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 3.

Integrated intensity of ¹³CO (J = 1 − 0). Left: ¹³CO integrated intensity of a simulated bubble without noise. Middle: ¹³CO integrated intensity of a simulated bubble convolved with a beam of size 50″ and with 0.125 K noise. Right: ¹³CO integrated intensity of an observed bubble, TMB 8, identified by Li et al. (2015).

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