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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 2.

ALMA 1.3 mm continuum map of I19368. The dashed gray contours delineate the boundaries of the southern filament region and the northern filament region. Left: 15 dense cores are marked with ellipses. Seven fragments (frags 1–7) are indicated with unfilled diamonds. Right: The solid black contours are [3, 5, 10, 20, 40, 80, 160] × σrms (σrms = 0.10 mJy beam−1). Green stars and blue crosses represent the protostellar and prestellar cores, respectively. The green diamonds indicate seven fragments same as the left panel. The synthesized beam and a 0.1 pc scale bar are shown in the lower left and the upper right corners, respectively.

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