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.
Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation
2 Pith papers cite this work, alongside 327 external citations. Polarity classification is still indexing.
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Type Ib supernovae are systematically bluer at optical peak than Type Ic supernovae, suggesting their progenitors contain more helium.
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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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Type Ib supernovae are bluer than Type Ic supernovae
Type Ib supernovae are systematically bluer at optical peak than Type Ic supernovae, suggesting their progenitors contain more helium.