Image Details

Choose export citation format:

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 4.

Models explaining the kinematics of gas around G336.01–0.82 from CH3OH ﹩{J}_{{K}_{a},{K}_{c}}={18}_{\mathrm{3,15}}-{17}_{\mathrm{4,14}}\,A,{v}_{t}=0﹩ emission in position-position–velocity space. This figure is available online as an interactive figure. The blue surface layers show the CH3OH emission levels of 5–15 × σ rms in steps of 2.5 with σ rms = 2.6 mJy beam−1. (a) IRE model surface layers at the same emission levels. (b) Spatial projection of the streamer models. In the interactive version, the velocity dimension can be explored and the models plotted enabled/disabled. The coordinates are with respect to ALMA1 (indicated with a yellow sphere: 16h35m09.ˢ261, −48°46′47.″659, −47.2 km s−1). The green lines indicate the projection of the zero offsets on each axis.

(An interactive version of this figure is available.)

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

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse