29 September 2026 to 3 October 2026
Africa/Johannesburg timezone

Magnetic Regulation and Energetic Stellar Feedback in Massive Galactic Star-Forming Regions

2 Oct 2026, 11:53
12m
Contributed Talk Other High-Energy Sources Other High-Energy Sources 1

Speaker

PATRICK OKEZUONU (ABIA STATE UNIVERSITY, UTURU)

Description

Energetic feedback from massive young stars can modify the same magnetic structures that regulate gravitational collapse, yet the observational connection between feedback-driven magnetic restructuring and star-formation efficiency (SFE) remains poorly constrained. We investigate 11 high-mass Galactic star-forming regions observed with the James Clerk Maxwell Telescope (JCMT), combining plane-of-sky magnetic-field strength, magnetic morphology, normalized mass-to-flux ratio, magnetic criticality, SFE, and published evidence for feedback–magnetic-field interaction. Magnetic-field strengths span 138.83 – 3364.93 μG, while 10 of the 11 regions (90.9%) are magnetically supercritical, indicating that gravitational collapse can proceed despite moderate-to-strong fields. Magnetic-field strength shows only a weak, statistically insignificant relation with SFE (ρ=-0.191), (p=0.573), while the mass-to-flux ratio exhibits a stronger but non-significant association (ρ=-0.419), (p=0.199). Source-by-source polarization studies reveal direct observational evidence of feedback-driven magnetic-field restructuring in four regions and suggestive evidence in three additional sources, including field alignment with outflow cavities, shock-related distortion, and reorientation by ionized or explosive feedback. Regions with direct feedback–magnetic interaction have a median SFE of 0.00721, compared with 0.0375 for sources in which such interaction is not observationally established. Although the small sample precludes a causal interpretation, the result provides a direct observational link between feedback environment, magnetic-field response, and star-formation activity. The findings favour a coupled evolutionary framework in which gravitational collapse proceeds predominantly in supercritical magnetized gas, stellar feedback subsequently reshapes the magnetic environment, and the resulting star-formation efficiency reflects the combined action of gravity, magnetic regulation, and energetic feedback rather than magnetic-field strength alone.

Authors

Mr CHINEDU OBED DIKE (Alex Ekwueme Federal University, Ndufu-Alike, Nigeria) Mr IFEANYICHUKWU DAVID OYOR (Akanu Ibiam Federal Polytechnic Unwana, Ebonyi State, Nigeria) Prof. IKECHUKWU UGOCHUKWU CHIEMEKA (ABIA STATE UNIVERSITY, UTURU) Prof. JEMIMA NGOZI OGWO (ABIA STATE UNIVERSITY, UTURU) PATRICK OKEZUONU (ABIA STATE UNIVERSITY, UTURU) Dr PRINCE ORJI ORJI (University of Nigeria, Nsukka, Nigeria.)

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