First ALMA observations of the Arches cluster yield mass-loss rates for WN and O stars plus evidence for radially decreasing wind clumping from combined radio-mm spectral indices.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
Advocates for a 2deg x 0.4deg multi-wavelength SKA-Mid continuum survey plus decade-long monitoring of the Galactic Centre nuclear star cluster to address multiple science questions with one dataset.
citing papers explorer
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ALMA measurements of mass loss and wind clumping in the massive stars of the Arches cluster
First ALMA observations of the Arches cluster yield mass-loss rates for WN and O stars plus evidence for radially decreasing wind clumping from combined radio-mm spectral indices.
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The Nearest Galactic Nucleus: Studying the Galactic Centre with SKA-Mid
Advocates for a 2deg x 0.4deg multi-wavelength SKA-Mid continuum survey plus decade-long monitoring of the Galactic Centre nuclear star cluster to address multiple science questions with one dataset.