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ALMA Band 9 CO(6–5) Reveals a Warm Ring Structure Associated with the Embedded Protostar in the Cold Dense Core MC 27/L1521F

  • Authors: Kazuki Tokuda, Mitsuki Omura, Naoto Harada, Ayumu Shoshi, Naofumi Fukaya, Toshikazu Onishi, Kengo Tachihara, Kazuya Saigo, Tomoaki Matsumoto, Yasuo Fukui, Akiko Kawamura, Masahiro N. Machida

Kazuki Tokuda et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 3.

Channel maps of the CO(J = 6–5) emission at the native spectral resolution (Δv = 0.12 km s−1), shown as a 3 × 3 panel. All panels are displayed in brightness temperature units (K). The central velocity channel is shown in the upper right corners of each panel in km s−1 units. The beam size of ﹩1\mathop{.}\limits{^{\prime\prime} }8\times 1\mathop{.}\limits{^{\prime\prime} }3﹩ (Position Angle ﹩=\,-6\mathop{.}\limits^{^\circ }1﹩) is shown in the ellipse at the lower left corner in the lower left panel. The red cross shows the position of the protostar.

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