Detection of HC3N Maser Emission in NGC 253

Simon P. Ellingsen, Xi Chen, Shari L. Breen, Hai Hua Qiao

Research output: Contribution to journalArticlepeer-review

9 Citations (Scopus)

Abstract

We report the detection of maser emission from the J = 4-3 transition of HC3N at 36.4 GHz toward the nearby starburst galaxy NGC 253. This is the first detection of maser emission from this transition in either a Galactic or extragalactic source. The HC3N maser emission has a brightness temperature in excess of 2500 K and is offset from the center of the galaxy by approximately 18′ (300 pc), but close to a previously reported class I methanol maser. Both the HC3N and methanol masers appear to arise near the interface between the galactic bar and the central molecular zone, where it is thought that molecular gas is being transported inwards, producing a region of extensive low-velocity shocks.

Original languageEnglish
Article numberL14
JournalAstrophysical Journal Letters
Volume841
Issue number1
DOIs
Publication statusPublished - 20 May 2017
Externally publishedYes

Fingerprint

Dive into the research topics of 'Detection of HC3N Maser Emission in NGC 253'. Together they form a unique fingerprint.

Cite this