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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Theoretical predictions for local BBH merger rates exceed observations by a factor >10 under conservative SFRD and metallicity assumptions, indicating need for revisions in stellar evolution.
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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Can current models predict the local black hole merger rate?
Theoretical predictions for local BBH merger rates exceed observations by a factor >10 under conservative SFRD and metallicity assumptions, indicating need for revisions in stellar evolution.