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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 6.

Maps derived from the VLA NH3 observations overlaid with the contours of ALMA 1.3 mm continuum emission. (a) Velocity field (moment 1) map of NH3 (1, 1) main hyperfine line. The northern filament and the southern filament are velocity-coherent. (b) Rotational temperature map. (c) FWHM map of NH3 (1, 1) main hyperfine line. In all panels, the contours are [3, 5, 10, 20, 40, 80, 160] × σrms (σrms = 0.10 mJy beam−1). The synthesized beam of 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩68 × 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩58 is shown in the lower left of each panel, and a 0.1 pc scale is in the upper right in panel (c).

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