Diversity of SEDs among the Star Forming Regions in NGC 1365
Stephen Hannon·Kathryn Kreckel·Hamid Hassani·Jessica Sutter·J. L. Rodriguez·Bradley C Whitmore·David A Thilker·Daniel A Dale·Janice C Lee·Thomas G Williams·Daizhong Liu·Erik Rosolowsky·Ralf S. Klessen·Kathryn Grasha·Rémy Indebetouw·Médéric Boquien·Kiana F. Henny·Eva Schinnerer·Aida Wofford
Abstract Studying samples of young star-forming regions allows us to statistically examine the evolution of their natal gas and dust along with the associated timescales in the volatile early stages of their lives. With the PHANGS survey data, we analyze the diversity of spectral energy distributions (SEDs) for the rich sample of massive star-forming regions found in NGC 1365. By combining unique detections across a variety of datasets from HST, JWST, and ALMA images, we produce a catalog of 85