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Adv."],"published-print":{"date-parts":[[2026,9,4]]},"abstract":"<jats:p>\n                    Feedback from massive stars regulates the formation of next-generation stars and planets and thus shapes the evolution of galaxies, yet observational evidence capable of determining which mechanism dominates the feedback process has long been lacking. Here, we present a large-scale H\n                    <jats:sub>I<\/jats:sub>\n                    survey toward Orion A. With an unprecedented sensitivity and superior resolution, FAST (Five-hundred-meter Aperture Spherical radio Telescope) reveals a well-defined heart-shaped expanding H\n                    <jats:sub>I<\/jats:sub>\n                    bubble, enshrouding the well-known \u201cVeil\u201d bubble of ionized gas. The photoionization-driven and wind-driven gas expands at 10.9 and 13.8 kilometers per second, respectively, with a kinetic energy ratio of 1:2 assuming a spherical symmetry and a uniform H\n                    <jats:sub>I<\/jats:sub>\n                    -to-H\n                    <jats:sub>2<\/jats:sub>\n                    ratio. This first direct comparison within a single bubble shows that radiation does not dominate the feedback process as predicted by classical theories; instead, stellar winds contribute a comparable share of the injected kinetic energy.\n                  <\/jats:p>","DOI":"10.1126\/sciadv.aec0787","type":"journal-article","created":{"date-parts":[[2026,9,4]],"date-time":"2026-09-04T17:58:46Z","timestamp":1788544726000},"update-policy":"https:\/\/doi.org\/10.34133\/aaas_crossmark","source":"Crossref","is-referenced-by-count":0,"title":["Identifying the principal mechanism of star formation feedback"],"prefix":"10.1126","volume":"12","author":[{"ORCID":"https:\/\/orcid.org\/0000-0003-2218-3437","authenticated-orcid":true,"given":"Chong","family":"Li","sequence":"first","affiliation":[{"name":"Purple Mountain Observatory and Key Laboratory of Radio Astronomy, CAS, Nanjing 210033, 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