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36 GHz methanol lines from nearby galaxies: maser or quasi-thermal emission?

Humire, P., Henkel, C., Gong, Y., Leurini, S., Mauersberger, R., Levshakov, S., et al. (2020). 36 GHz methanol lines from nearby galaxies: maser or quasi-thermal emission? åp, 633: A106, pp. A106. doi:10.1051/0004-6361/201936330.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0008-42EB-5 Version Permalink: https://hdl.handle.net/21.11116/0000-0008-42EC-4

Genre: Journal Article

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Creators:
Humire, P.K.¹, Author
Henkel, C.¹, Author
Gong, Y.¹, Author
Leurini, S.¹, Author
Mauersberger, R.¹, Author
Levshakov, S.A., Author
Winkel, B.¹, Author
Tarchi, A., Author
Castangia, P., Author
Malawi, A., Author
Asiri, H., Author
Ellingsen, S.P., Author
McCarthy, T.P., Author
Chen, X., Author
Tang, X., Author

Affiliations:
1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652

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Free keywords: masers, galaxies: spiral, galaxies: individual: IC 342, galaxies: individual: Maffei 2, galaxies: ISM, radio lines: galaxies, Astrophysics - Astrophysics of Galaxies

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Dates: Date issued: 2020-01

Publication Status: Issued

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Identifiers: DOI: 10.1051/0004-6361/201936330
BibTex Citekey: 2020A&A...633A.106H

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Title: åp

Source Genre: Journal

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Pages: - Volume / Issue: 633 Sequence Number: A106 Start / End Page: A106 Identifier: -