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FAST Observations of Filamentary and Compact H I Structure in the Magellanic Stream IV Field

  • Authors: Yuxin Xiao, 雨欣 肖, Qingzheng Yu, 清正 余, Taotao Fang, 陶陶 方, Di Li, 菂 李, Shulan Yan, 淑澜 鄢, Shuo Zhang, 硕 张

Yuxin Xiao et al 2026 The Astrophysical Journal 1011 .

  • Provider: AAS Journals

Caption: Figure 6.

Four representative individual-pixel spectra of the cataloged H I sources, together with the Gaussian fitting results. Only Gaussian components above threshold = 2 are shown. The original spectra are shown in black, with the best-fit in orange and independent Gaussian components in cyan, purple, and green. All spectra are fitted using the ROHSA model with N = 3. In the bottom row, the left panel shows an example that satisfies the adopted merging criteria, whereas the right panel shows an example that does not satisfy the merging criteria.

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