A turbulent stellar atmosphere in full view

Gail H. Schaefer ()
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Gail H. Schaefer: CHARA Array of Georgia State University

Nature, 2017, vol. 548, issue 7667, 288-289

Abstract: The dynamic motion of gas in the outer atmosphere of a red supergiant star has been mapped, providing clues to the mysterious mechanism that causes massive stars to lose mass through stellar winds. See Letter p.310

Date: 2017
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DOI: 10.1038/548288a

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