A review of red supergiant binary systems finds a flat mass-ratio distribution among 88 Small Magellanic Cloud candidates, but the assumptions used to infer those masses are shown to be too simplistic by new Hubble spectra.
(1956) Harvard Announcement Card, 1340
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Hot and cool: Characterising the companions of red supergiant stars in binary systems
A review of red supergiant binary systems finds a flat mass-ratio distribution among 88 Small Magellanic Cloud candidates, but the assumptions used to infer those masses are shown to be too simplistic by new Hubble spectra.