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Multiscale Mass-assembly Scenario in the High-mass Star-forming Filament IRAS 19368+2239 Observed as Part of the INFANT Survey

  • Authors: Chengzhi Meng, Hong-Li Liu, Xing Lu, Yu Cheng, R. Galván-Madrid, H. B. Liu, Q. Zhang, S. H. Li, A.E. Guzmán, P. Sanhueza, Kei E. I. Tanaka

Chengzhi Meng et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 8.

Velocity channel maps of the H2CO 3(0, 3)−2(0, 2) line emission above 3 rms (rms ∼ 1.53 Jy beam−1 m s−1) toward the I19368 region. The red dashed contours in each box are the same as in Figure 2, depicting the filament morphology. The corresponding LSR velocity of each channel map is displayed in the top right of each panel. The synthesized beam of 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩80 × 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩67 is shown in the lower left corner of each panel.

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