Class i Methanol Maser Emission in NGC 4945

Tiege P. McCarthy, Simon P. Ellingsen, Xi Chen, Shari L. Breen, Maxim A. Voronkov, Hai Hua Qiao

Research output: Contribution to journalArticlepeer-review

Abstract

We have detected maser emission from the 36.2 GHz (4-1 → 30E) methanol transition towards NGC 4945. This emission has been observed in two separate epochs and is approximately five orders of magnitude more luminous than typical emission from this transition within our Galaxy. NGC 4945 is only the fourth extragalactic source observed hosting class I methanol maser emission. Extragalactic class I methanol masers do not appear to be simply highly-luminous variants of their galactic counterparts and instead appear to trace large-scale regions where low-velocity shocks are present in molecular gas.

Original languageEnglish
Pages (from-to)105-108
Number of pages4
JournalProceedings of the International Astronomical Union
Volume13
Issue numberS336
DOIs
Publication statusPublished - 2017
Externally publishedYes

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