The paper makes a quantified case that a diffraction-limited ultraviolet integral field spectrograph on HWO (5 mas, R about 2000) would resolve and characterize very massive stars in nearby starbursts.
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Very Massive Stars with the Habitable Worlds Observatory
The paper makes a quantified case that a diffraction-limited ultraviolet integral field spectrograph on HWO (5 mas, R about 2000) would resolve and characterize very massive stars in nearby starbursts.