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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 9.

Results of identified filamentary skeletons for the I19368 region. The background shows the integrated intensity map of H2CO 3(0, 3)−2(0, 2) line for the velocity channel centered at 35.5 km s−1. The dashed contour outlining the northern and the southern filamentary segments is the same as in Figure 2. The red skeletons show the 2 long filamentary structures (L1 and L2), and the orange branches indicate the 18 dense striations tagged 1−18. The synthesized beam of 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩80 × 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩67 and a 0.1 pc scale bar are located in the lower left and the upper right corners, respectively.

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