The Large-Scale Atomic and Molecular Gas in the Circinus Galaxy
S. J. Curran, B. S. Koribalski, I. Bains

TL;DR
This study maps atomic and molecular gas in the Circinus galaxy, revealing gas distribution, kinematics, and mass ratios, and providing insights into its structure, starburst activity, and dark matter content.
Contribution
First detailed large-scale atomic and molecular gas map of Circinus, analyzing gas distribution, kinematics, and mass ratios to understand galaxy dynamics and starburst regions.
Findings
Molecular gas mass ~2 billion solar masses.
Atomic gas mass ~6 billion solar masses.
Steep rotation curve dip at ~1 kpc.
Abstract
We have used the ATCA and the SEST to map the large-scale atomic and molecular gas in the nearby Circinus galaxy. The HI mosaic of Circinus exhibits the warps in position angle and inclination revealed in the single-pointing image, both of which appear to settle beyond the inner 30 kpc which was previously imaged. The molecular gas has been mapped in both the CO transitions, where we derive a total molecular gas mass of ~2e9 Mo. Within a radius of 3 kpc, i.e. where CO was clearly detected, the molecular fraction climbs steeply from ~0.7 to unity with proximity to the nucleus. Our HI mosaic gives an atomic gas mass of ~6e9 Mo which is 70% of the fully mapped single dish value. The total neutral gas mass to dynamical mass ratio is therefore 3%, consistent with the SAS3 classification of Circinus. The high (molecular) gas mass fraction found previously, only occurs close to the central…
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