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Star Formation Drives Production of Low-energy Cosmic Rays

  • Authors: Ningyu Tang, Jiahao Liu, Di Li, Ruizhi Yang, Thomas G. Bisbas, Bing Liu, Marko Krčo, Paul Goldsmith, Paola Caselli, Sihan Jiao, Yan Gong, Gan Luo, Xinwen Shu, Liangchong Zhu, Xiaohui Sun, Chen Wang, Tao-Chung Ching, Donghui Quan, Junzhi Wang, Xuejian Jiang, Pei Zuo

Ningyu Tang et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 2.

Fitting profile of HINSA toward the positions A–E shown in Figure 1. The top panel shows the observed H I spectrum (black) and the recovered H I spectrum without self-absorption (red). The middle panel displays the HINSA profile. The 13CO(1–0) spectrum, Gaussian fitting components, and the overall fitting profile are shown as solid black, solid gray, and red dashed lines, respectively, in the lower panel.

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