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PHANGS–JWST First Results: Rapid Evolution of Star Formation in the Central Molecular Gas Ring of NGC 1365


Abstract Large-scale bars can fuel galaxy centers with molecular gas, often leading to the development of dense ring-like structures where intense star formation occurs, forming a very different environment compared to galactic disks. We pair ~0.3" (30pc) resolution new JWST/MIRI imaging with archival ALMA CO(2-1) mapping of the central ~5kpc of the nearby barred spiral galaxy NGC1365, to investigate the physical mechanisms responsible for this extreme star formation. The molecular gas morphology is resolved into two well-known bright bar lanes that surround a smooth dynamically cold gas disk (R_gal ~ 475pc) reminiscent of non-star-forming disks in early type galaxies and likely fed by gas inflow triggered by stellar feedback in the lanes. The lanes host a large number of JWST-identified massive young star clusters. We find some evidence for temporal star formation evolution along the ring. The complex kinematics in the gas lanes reveal strong streaming motions and may be consistent with convergence of gas streamlines expected there. Indeed, the extreme line-widths are found to be the result of inter-`cloud' motion between gas peaks; ScousePy decomposition reveals multiple components with line widths of <sigma_CO,scouse> ~ 19km/s and surface densities of <Sigma_H2,scouse> ~ 800M_sun/pc^2, similar to the properties observed throughout the rest of the central molecular gas structure. Tailored hydro-dynamical simulations exhibit many of the observed properties and imply that the observed structures are transient and highly time-variable. From our study of NGC1365, we conclude that it is predominantly the high gas inflow triggered by the bar that is setting the star formation in its CMZ.
Authors E. Schinnerer ORCID , Éric Emsellem ORCID , Jonathan D. Henshaw ORCID , Daizhong Liu ORCID , Sharon E. Meidt ORCID , Miguel Querejeta ORCID , Florent Renaud ORCID , Mattia C. Sormani ORCID , Jiayi Sun ORCID , Oleg V. Egorov ORCID , Kirsten L. Larson ORCID , Adam K. Leroy ORCID , Erik Rosolowsky ORCID , Karin Sandström ORCID , Thomas G. Williams ORCID , Ashley T. Barnes ORCID , Frank Bigiel ORCID , Mélanie Chevance ORCID , Yixian Cao ORCID , Rupali Chandar ORCID , Daniel A. Dale University of WyomingORCID , Cosima Eibensteiner ORCID , Simon C. O. Glover ORCID , Kathryn Grasha ORCID , Stephen Hannon ORCID , Hamid Hassani ORCID , Jaeyeon Kim ORCID , Ralf S. Klessen ORCID , J. M. Diederik Kruijssen ORCID , E. J. Murphy ORCID , Justus Neumann ORCID , Hsi-An Pan ORCID , J. Pety ORCID , Tomoka Tosaki ORCID , Sophia K. Stuber ORCID , Robin G. Treß ORCID , A. Usero ORCID , Elizabeth J. Watkins ORCID , Bradley C. Whitmore ORCID
Journal Info IOP Publishing | The Astrophysical Journal Letters , vol: 944 , iss: 2 , pages: L15 - L15
Publication Date 2/1/2023
ISSN 2041-8205
TypeKeyword Image article
Open Access gold Gold Access
DOI https://doi.org/10.3847/2041-8213/acac9e
KeywordsKeyword Image Star Formation (Score: 0.496837)