Massive stars in the Milky Way form over Myr timescales that increase with final mass, inferred from joint LF fitting of compact HII regions and OB stars under the inertial-inflow model.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 2verdicts
UNVERDICTED 2representative citing papers
The Galactic Center Lobe is a foreground HII region at ~2 kpc, photoionized and forming a closed outer loop, not a Galactic center feature.
citing papers explorer
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Compact HII Regions as Clocks of Massive-Star Formation: Evidence for Long Formation Timescales
Massive stars in the Milky Way form over Myr timescales that increase with final mass, inferred from joint LF fitting of compact HII regions and OB stars under the inertial-inflow model.
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SDSS-V LVM: Verifying what, and where, the 'Galactic Center' Lobe is
The Galactic Center Lobe is a foreground HII region at ~2 kpc, photoionized and forming a closed outer loop, not a Galactic center feature.