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  Temperature Structure of the Pipe Nebula Studied by the Intensity Anomaly of the OH 18 cm Transition

Ebisawa, Y., Sakai, N., Menten, K. M., Oya, Y., & Yamamoto, S. (2020). Temperature Structure of the Pipe Nebula Studied by the Intensity Anomaly of the OH 18 cm Transition. \apj, 904(2): 136, pp. 136. doi:10.3847/1538-4357/abc16f.

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 Creators:
Ebisawa, Yuji, Author
Sakai, Nami, Author
Menten, Karl M.1, Author
Oya, Yoko, Author
Yamamoto, Satoshi, Author
Affiliations:
1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652              

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Free keywords: Molecular clouds, Interstellar molecules, 1072, 849, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
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 Dates: 2020-12
 Publication Status: Issued
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 Identifiers: DOI: 10.3847/1538-4357/abc16f
BibTex Citekey: 2020ApJ...904..136E
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Title: \apj
Source Genre: Journal
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Pages: - Volume / Issue: 904 (2) Sequence Number: 136 Start / End Page: 136 Identifier: -