arXiv · 0809.4605
The Antares emission nebula and mass loss of alpha Sco A
Abstract
The Antares nebula is a peculiar emission nebula seen in numerous Fe II lines and in radio free-free emission, probably associated with the H II region caused by alpha Sco B in the wind of alpha Sco A. High-resolution spectra with spatial resolution were used to study the emission line spectrum, the physical nature of the nebula and to determine the mass-loss rate of the M supergiant alpha Sco A.
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D. Reimers, H. -J. Hagen, R. Baade, K. Braun. 2008-09-26. The Antares emission nebula and mass loss of alpha Sco A. https://doi.org/10.1051/0004-6361:200809983
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