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Digging into the Interior of Hot Cores with ALMA: Spiral Accretion into the High-mass Protostellar Core G336.01–0.82

  • Authors: Fernando A. Olguin, Patricio Sanhueza, Huei-Ru Vivien Chen, Xing Lu, Yoko Oya, Qizhou Zhang, Adam Ginsburg, Kotomi Taniguchi, Shanghuo Li, Kaho Morii, Takeshi Sakai, Fumitaka Nakamura

Fernando A. Olguin et al 2023 The Astrophysical Journal Letters 959 .

  • Provider: AAS Journals

Caption: Figure 8.

Standard deviation map of CH3CN J = 12 − 11 peak brightness temperature for K transitions 2 to 4. Gray contours show the continuum emission at the same levels as in Figure 1, and the green triangles indicate the continuum peaks. The beam size ellipse is shown in the lower left corner.

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