| Original language | English |
|---|---|
| Pages (from-to) | 2445–2462 |
| Number of pages | 18 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 538 |
| Issue number | 4 |
| Early online date | 19 Mar 2025 |
| DOIs | |
| Publication status | E-pub ahead of print - 19 Mar 2025 |
Data Availability Statement
The raw CO(1-0) data of the disc used for this work are available on the IRAM data archive.4 The CO(3-2) data in the disc are available on the HASHTAG archive.5 The CO(1-0) and CO(3-2) data in the nuclear ring used for this work are available upon request to the corresponding author.Funding
This work was supported by the National Key R&D Program of China for grant 2022YFA1605300, the National Natural Science Foundation of China (grant 11988101 and 12225302) and the National Key Research and Development Programme of China (no. 2022YFA1605000 and no. 2022YFF0503402). ZNL acknowledges support by the China National Postdoctoral Programme for Innovation Talents (grant BX20220301) and the East Asian Core Observatories Association Fellowship. JW thank the support from National Natural Science Foundation of China (grant 12041302) and National Key Research and Development Programme of China (no. 2023YFA1608004). RG was supported in part by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. BL acknowledges support by the National Research Foundation of Korea (NRF), grant nos. 2022R1A2C100298213. DL is a New Cornerstone investigator.