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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 1.

Integrated intensity of H I (panel (a)) and 13CO(1–0) (panel (b)) toward the Orion region. The velocity range is from 0 to 15 km s−1 and a correction for the main beam efficiency has been adopted. The positions of well known clouds and stars are shown in panel (b). The distribution of young stellar objects overlaid on the Herschel extinction map is displayed in panel (c). The boundaries of the five subregions are delineated by white dashed lines, and the five positions A–E covering regions with different environments are indicated by magenta dots. Yellow dots indicate the positions of young stellar objects.

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