ACA CO(J = 2-1) Mapping of the Nearest Spiral Galaxy M33. I. Initial Results and Identification of Molecular Clouds
Abstract
We present the results of ALMA-ACA 7 m array observations in 12CO(J = 2-1), 13CO(J = 2-1), and C18O(J = 2-1) line emission toward the molecular-gas disk in the Local Group spiral galaxy M33 at an angular resolution of 7.″31 × 6.″50 (30 × 26 pc). We combined the ACA 7 m array 12CO(J = 2-1) data with the IRAM 30 m data to compensate for emission from diffuse molecular-gas components. The ACA+IRAM combined 12CO(J = 2-1) map clearly depicts the cloud-scale molecular-gas structure over the M33 disk. Based on the ACA+IRAM 12CO(J = 2-1) cube data, we cataloged 848 molecular clouds with a mass range from 103-106 M ⊙. We found that high-mass clouds (≥105 M ⊙) tend to associate with the 8 μm bright sources in the spiral arm region, while low-mass clouds (<105 M ⊙) tend to be apart from such 8 μm bright sources and to exist in the inter-arm region. We compared the cataloged clouds with GMCs observed by the IRAM 30 m telescope at 49 pc resolution (IRAM GMC), and found that a small IRAM GMC is likely to be identified as a single molecular cloud even in ACA+IRAM CO data, while a large IRAM GMC can be resolved into multiple ACA+IRAM clouds. The velocity dispersion of a large IRAM GMC is mainly dominated by the line-of-sight velocity difference between small clouds inside the GMC rather than the internal cloud velocity broadening.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- August 2023
- DOI:
- 10.3847/1538-4357/ace4bd
- arXiv:
- arXiv:2307.02039
- Bibcode:
- 2023ApJ...953..164M
- Keywords:
-
- Triangulum Galaxy;
- Local Group;
- Molecular clouds;
- Interstellar medium;
- 1712;
- 929;
- 1072;
- 847;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 23 pages, 17 figures, accepted for publication in the Astrophysical Journal