The Formation of Milky Way “Bones”: Ubiquitous HI Narrow Self-absorption Associated with CO Emission

Shenglan Sun, Ke Wang, Xunchuan Liu, Fengwei Xu

Open source

DOI: 10.3847/2041-8213/ad77ce
Published: 2024-09-01
Container: The Astrophysical Journal Letters
Publisher: American Astronomical Society
Open access: unknown

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Cite this work

BibTeX

@article{allodium:10.3847/2041-8213/ad77ce,
  title = {The Formation of Milky Way “Bones”: Ubiquitous HI Narrow Self-absorption Associated with CO Emission},
  author = {Shenglan Sun and Ke Wang and Xunchuan Liu and Fengwei Xu},
  year = {2024},
  journal = {The Astrophysical Journal Letters},
  doi = {10.3847/2041-8213/ad77ce},
  url = {https://doi.org/10.3847/2041-8213/ad77ce}
}

RIS

TY  - JOUR
TI  - The Formation of Milky Way “Bones”: Ubiquitous HI Narrow Self-absorption Associated with CO Emission
AU  - Shenglan Sun
AU  - Ke Wang
AU  - Xunchuan Liu
AU  - Fengwei Xu
PY  - 2024
JO  - The Astrophysical Journal Letters
DO  - 10.3847/2041-8213/ad77ce
UR  - https://doi.org/10.3847/2041-8213/ad77ce
ER  -

APA

Sun, S., Wang, K., Liu, X., & Xu, F. (2024). The Formation of Milky Way “Bones”: Ubiquitous HI Narrow Self-absorption Associated with CO Emission. The Astrophysical Journal Letters. https://doi.org/10.3847/2041-8213/ad77ce

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crossref · retrieved 2026-09-26T06:53:09.952Z