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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 5.

Average peak brightness temperature from CH3CN J = 12 − 11 K transitions 2 to 4. The blue and red regions in (a) indicate where the properties in Section 4.2 are estimated and roughly follow the continuum 5σ level. Gray contours show the continuum emission from the combined data at the same levels as in Figure 1 but with σ rms = 54 μJy beam−1, and the green triangles indicate the continuum peaks. The beam size ellipse is shown in the lower left corner.

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