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

MPS-Authors

Humire,  P.K.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Henkel,  C.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Gong,  Y.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Leurini,  S.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Mauersberger,  R.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Winkel,  B.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Citation

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.


Cite as: https://hdl.handle.net/21.11116/0000-0008-42EB-5
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