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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 1.

ALMA maps of G336.01–0.82. (a) Continuum map at 1.3 mm. The position of the three local continuum peaks is indicated by the green labeled triangles. The contour levels are −3, 5, 10, 20, 40, 80 × σ rms with σ rms = 55 μJy beam−1. (b) HC3N J = 24 − 23 l = 1f, v 7 = 1 zeroth moment map contours over the continuum map. The contours are 5, 8, 10, 15, 20, 25 × σ rms with σ rms = 11 mJy beam−1 km s−1. (c) SiO J = 5–4 blue- and redshifted, and the contour levels are 5, 6, 7 ... 12 × σ rms with σ rms = 7.7 mJy beam−1 km s−1. Velocity integration ranges with respect to the systemic velocity are annotated by the respective color. The beam size of the continuum map is shown in the lower left corner.

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