Image Details

Choose export citation format:

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 5.

Velocity gradients ∇VLSR,∣∣ as a function of the filamentary structure length Lf. The black squares represent the density structures (16 striations and 2 long filamentary structures) in the I19368 region. Unfilled marks represent filamentary structure samples from A. Hacar et al. (2023). The green dashed line indicates the inverse relationship.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse