Discovery of a Giant Molecular Loop in the Central Region of NGC 253

NGC 253 is a starburst galaxy of SAB(s)c type with increasing interest because of its high activity at unrivaled closeness. Its energetic event is manifested as the vertical gas features in its central molecular zone, for which stellar feedback was proposed as the driving engine. In order to pursue details of the activity, we have undertaken a kinematic analysis of the ALMA archive data of (CO)-C-12(J = 3 - 2) emission at the highest resolution similar to 3 pc. We revealed that one of the non-rotating gas components in the central molecular zone shows a loop-like structure of similar to 200 pc radius. The loop-like structure is associated with a star cluster, whereas the cluster is not inside the loop-like structure and is not likely as the driver of the loop-like structure formation. Further, we find that the bar potential of NGC 253 seems to be too weak to drive the gas motion by the eccentric orbit. As an alternative, we frame a scenario that magnetic acceleration by the Parker instability is responsible for the creation of the loop-like structure. We show that the observed loop-like structure properties are similar to those in the Milky Way, and argue that recent magneto-hydrodynamics simulations lend support for the picture having the magnetic field strength of greater than or similar to 100 mu G. We suggest that cluster formation was triggered by the falling gas to the footpoint of the loop, which is consistent with a typical dynamical timescale of the loop similar to 1 Myr.

Automated summary

NGC 253 is a starburst galaxy with high activity in its central molecular zone. An analysis of the data revealed a loop-like structure associated with a star cluster. The weak bar potential of NGC 253 suggests that magnetic acceleration may be responsible for the creation of this structure.