New catalogue of 1327 extended Galactic HII regions from SMGPS 1.3 GHz data with distances, N_Ly fluxes, spectral types B3-O4, and reported correlations between radius, density, and ionizing luminosity.
Massive Star Birth: A Crossroads of Astrophysics , year = 2005, editor =
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The paper outlines the goals for the SKA-Mid Galactic Plane survey at 10-15 GHz to deliver the first uniform high-resolution view of ionized structures and feedback in the Milky Way.
Observational study of G12.79+0.43 identifies YSOs and HII regions powered by B-type stars and associates the complex with the rim of a molecular superbubble of diameter ~50 pc and expansion age ~0.3 Myr without establishing causality.
VLA imaging and modeling of five HC HII candidates indicate most are small UC HII regions, with G40.28-0.22 as the strongest remaining HC case.
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
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SMGPS: A study of Galactic HII regions with extended morphology
New catalogue of 1327 extended Galactic HII regions from SMGPS 1.3 GHz data with distances, N_Ly fluxes, spectral types B3-O4, and reported correlations between radius, density, and ionizing luminosity.
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The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO
The paper outlines the goals for the SKA-Mid Galactic Plane survey at 10-15 GHz to deliver the first uniform high-resolution view of ionized structures and feedback in the Milky Way.
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Star Formation at the Periphery of a Molecular Superbubble: The Case of G12.79+0.43
Observational study of G12.79+0.43 identifies YSOs and HII regions powered by B-type stars and associates the complex with the rim of a molecular superbubble of diameter ~50 pc and expansion age ~0.3 Myr without establishing causality.
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Physical characterization and modeling of candidate Hyper-Compact HII Regions
VLA imaging and modeling of five HC HII candidates indicate most are small UC HII regions, with G40.28-0.22 as the strongest remaining HC case.
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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.