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.
Title resolution pending
5 Pith papers cite this work, alongside 830 external citations. Polarity classification is still indexing.
5
Pith papers citing it
830
external citations · OpenAlex
years
2026 5representative citing papers
ALMA comparison finds starless cores in evolved IRBCs have ~2x higher median mass and density than in early IRDCs, favoring competitive accretion over massive prestellar core models for high-mass star formation.
MeerKAT radio data yield a catalogue of 1,327 extended Galactic HII regions with distances and ionising-photon fluxes, plus power-law scaling relations between luminosity, density, and radius.
SKA-Mid is predicted to yield samples of 10-100 low-metallicity Lyman continuum emitting galaxies per square degree, enabling multi-wavelength studies of feedback processes linked to ionizing photon escape.
This review summarizes the role of massive star feedback and projects how SKA radio observations will advance studies of HII regions, stellar winds, cosmic ray acceleration, and magnetic fields.
citing papers explorer
-
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.
-
Evolution of starless cores in massive clumps seen by the ALMA ASHES and QUARKS surveys
ALMA comparison finds starless cores in evolved IRBCs have ~2x higher median mass and density than in early IRDCs, favoring competitive accretion over massive prestellar core models for high-mass star formation.
-
SMGPS: A study of Galactic HII regions with extended morphology
MeerKAT radio data yield a catalogue of 1,327 extended Galactic HII regions with distances and ionising-photon fluxes, plus power-law scaling relations between luminosity, density, and radius.
-
Probing the Nature of Lyman Continuum Emitting and Low-metallicity Galaxies Using the SKA
SKA-Mid is predicted to yield samples of 10-100 low-metallicity Lyman continuum emitting galaxies per square degree, enabling multi-wavelength studies of feedback processes linked to ionizing photon escape.
-
The Impact and Environment of Massive Stars and Stellar Clusters
This review summarizes the role of massive star feedback and projects how SKA radio observations will advance studies of HII regions, stellar winds, cosmic ray acceleration, and magnetic fields.