Detailed Record



PHANGS–JWST First Results: A Statistical View on Bubble Evolution in NGC 628


Abstract The first JWST observations of nearby galaxies have unveiled a rich population of bubbles that trace the stellar-feedback mechanisms responsible for their creation. Studying these bubbles therefore allows us to chart the interaction between stellar feedback and the interstellar medium, and the larger galactic flows needed to regulate star formation processes globally. We present the first catalog of bubbles in NGC 628, visually identified using Mid-Infrared Instrument F770W Physics at High Angular resolution in Nearby GalaxieS (PHANGS)–JWST observations, and use them to statistically evaluate bubble characteristics. We classify 1694 structures as bubbles with radii between 6 and 552 pc. Of these, 31% contain at least one smaller bubble at their edge, indicating that previous generations of star formation have a local impact on where new stars form. On large scales, most bubbles lie near a spiral arm, and their radii increase downstream compared to upstream. Furthermore, bubbles are elongated in a similar direction to the spiral-arm ridgeline. These azimuthal trends demonstrate that star formation is intimately connected to the spiral-arm passage. Finally, the bubble size distribution follows a power law of index p = −2.2 ± 0.1, which is slightly shallower than the theoretical value by 1–3.5 σ that did not include bubble mergers. The fraction of bubbles identified within the shells of larger bubbles suggests that bubble merging is a common process. Our analysis therefore allows us to quantify the number of star-forming regions that are influenced by an earlier generation, and the role feedback processes have in setting the global star formation rate. With the full PHANGS–JWST sample, we can do this for more galaxies.
Authors Elizabeth J. Watkins ORCID , Ashley T. Barnes ORCID , Kiana F. Henny University of WyomingORCID , Hwi Kim ORCID , Kathryn Kreckel ORCID , Sharon E. Meidt ORCID , Ralf S. Klessen ORCID , Simon C. O. Glover ORCID , Thomas G. Williams ORCID , Ben Keller ORCID , Adam K. Leroy ORCID , Erik Rosolowsky ORCID , M. Boquien ORCID , Gagandeep S. Anand ORCID , Francesco Belfiore ORCID , Frank Bigiel ORCID , Guillermo A. Blanc ORCID , M. Boquien ORCID , Yixian Cao ORCID , Rupali Chandar ORCID , Ness Mayker Chen ORCID , Mélanie Chevance ORCID , Enrico Congiu ORCID , Daniel A. Dale University of WyomingORCID , Sinan Deger ORCID , Oleg V. Egorov ORCID , Éric Emsellem ORCID , Christopher M. Faesi ORCID , Kathryn Grasha ORCID , Brent Groves ORCID , Hamid Hassani ORCID , Jonathan D. Henshaw ORCID , Cinthya N. Herrera ORCID , Annie Hughes ORCID , Sarah Jeffreson ORCID , María J. Jiménez-Donaire ORCID , Eric W. Koch ORCID , J. M. Diederik Kruijssen ORCID , Kirsten L. Larson ORCID , Daizhong Liu ORCID , Laura A. Lopez ORCID , Ismael Pessa ORCID , J. Pety ORCID , Miguel Querejeta ORCID , Tomoka Tosaki ORCID , Karin Sandström ORCID , Fabian Scheuermann ORCID , E. Schinnerer ORCID , Mattia C. Sormani ORCID , Sophia K. Stuber ORCID , David A. Thilker ORCID , A. Usero ORCID , Bradley C. Whitmore ORCID
Journal Info IOP Publishing | The Astrophysical Journal Letters , vol: 944 , iss: 2 , pages: L24 - L24
Publication Date 2/1/2023
ISSN 2041-8205
TypeKeyword Image article
Open Access gold Gold Access
DOI https://doi.org/10.3847/2041-8213/aca6e4
KeywordsKeyword Image Young Stellar Objects (Score: 0.490128)