SED fitting of star clusters in NGC 628 identifies an evolutionary sequence from embedded young clusters to visible ones with a photo-dissociation region clearing timescale of approximately 4 Myr.
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3 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 3years
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UNVERDICTED 3representative citing papers
MHD simulations indicate that SKA-Mid Band 5a can detect filamentary polarized emission from ICM magnetic fields at high resolution and sensitivity, allowing inference of turbulence driving scales.
Simulations indicate SKAO AA4 surveys can trace ISM thermal and nonthermal processes in M51/NGC6946 analogs beyond z=2-3 in continuum and z=1 in HI, pointing to important nonthermal feedback at cosmic noon.
citing papers explorer
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Feedback in Extragalactic Star Clusters (FEAST): Spectral Energy Distributions and the Physical Properties of Star Clusters in NGC 628 with CIGALE
SED fitting of star clusters in NGC 628 identifies an evolutionary sequence from embedded young clusters to visible ones with a photo-dissociation region clearing timescale of approximately 4 Myr.
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Unraveling the Imprints of Fluctuation-dynamo on the Intracluster Medium with the SKA
MHD simulations indicate that SKA-Mid Band 5a can detect filamentary polarized emission from ICM magnetic fields at high resolution and sensitivity, allowing inference of turbulence driving scales.
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Unveiling the roles of thermal and nonthermal processes in the ISM & IGM structure formation and evolution of galaxies with SKAO
Simulations indicate SKAO AA4 surveys can trace ISM thermal and nonthermal processes in M51/NGC6946 analogs beyond z=2-3 in continuum and z=1 in HI, pointing to important nonthermal feedback at cosmic noon.