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PHANGS–JWST First Results: Multiwavelength View of Feedback-driven Bubbles (the Phantom Voids) across NGC 628


Abstract We present a high-resolution view of bubbles within The Phantom Galaxy (NGC 628); a nearby (~10Mpc), star-forming (~2Msun/yr), face-on (i~9deg) grand-design spiral galaxy. With new data obtained as part of the PHANGS-JWST treasury program, we perform a detailed case-study of two regions of interest, one of which contains the largest and most prominent bubble in the galaxy (The Phantom Void; over 1kpc in diameter), and the other being a smaller region that may be the precursor to such a large bubble (The Precursor Phantom Void). When comparing to matched resolution Halpha observations from the Hubble Space Telescope (HST), we see that the ionized gas is brightest in the shells of both bubbles, and is coincident with the youngest (~1Myr) and most massive (~100,000Msun) stellar associations. We also find an older generation (~20Myr) of stellar associations is present within the bubble of The Phantom Void. From our kinematic analysis of the HI, H2 (CO) and HII gas across The Phantom Void, we infer a high expansion speed of around 15 to 50km/s. The large size and high expansion speed of The Phantom Void suggest that the driving mechanism is sustained stellar feedback due to multiple mechanisms, where early feedback first cleared a bubble (as we observe now in The Precursor Phantom Void), and since then SNe have been exploding within the cavity, and have accelerated the shell. Finally, comparison to simulations shows a striking resemblance to our JWST observations, and suggests that such large-scale stellar feedback-driven bubbles should be common within other galaxies.
Authors Ashley T. Barnes ORCID , Elizabeth J. Watkins ORCID , Sharon E. Meidt ORCID , Kathryn Kreckel ORCID , Mattia C. Sormani ORCID , Robin G. Treß ORCID , Simon C. O. Glover ORCID , Frank Bigiel ORCID , Rupali Chandar ORCID , Éric Emsellem ORCID , Janice Lee ORCID , Adam K. Leroy ORCID , Karin Sandström ORCID , E. Schinnerer ORCID , Erik Rosolowsky ORCID , Francesco Belfiore ORCID , Guillermo A. Blanc ORCID , M. Boquien ORCID , Jakob S. den Brok ORCID , Yixian Cao ORCID , Mélanie Chevance ORCID , Daniel A. Dale University of WyomingORCID , Oleg V. Egorov ORCID , Cosima Eibensteiner ORCID , Kathryn Grasha ORCID , Brent Groves ORCID , Hamid Hassani ORCID , Jonathan D. Henshaw ORCID , Sarah Jeffreson ORCID , María J. Jiménez-Donaire ORCID , Ben Keller ORCID , Ralf S. Klessen ORCID , Eric W. Koch ORCID , J. M. Diederik Kruijssen ORCID , Kirsten L. Larson ORCID , Jing Li ORCID , Daizhong Liu ORCID , Laura A. Lopez ORCID , E. J. Murphy ORCID , Lukáš Neumann ORCID , J. Pety ORCID , Francesca Pinna ORCID , Miguel Querejeta ORCID , Florent Renaud ORCID , Tomoka Tosaki ORCID , Sumit K. Sarbadhicary ORCID , Amy Sardone ORCID , Rowan J. Smith ORCID , Sophia K. Stuber ORCID , Jiayi Sun ORCID , David A. Thilker ORCID , A. Usero ORCID , Bradley C. Whitmore ORCID , Thomas G. Williams ORCID
Journal Info IOP Publishing | The Astrophysical Journal Letters , vol: 944 , iss: 2 , pages: L22 - L22
Publication Date 2/1/2023
ISSN 2041-8205
TypeKeyword Image article
Open Access gold Gold Access
DOI https://doi.org/10.3847/2041-8213/aca7b9
KeywordsKeyword Image Young Stellar Objects (Score: 0.498249)