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The Antares emission nebula and mass loss of alpha Sco A

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arxiv 0809.4605 v1 pith:OPUX3XCO submitted 2008-09-26 astro-ph

D. Reimers , H.-J. Hagen , R. Baade , K. Braun This is my paper · ORCID
classification astro-ph
keywords alphaemissionnebulaantaresassociatedcauseddeterminefree-free
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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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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 25 citations worldwide. Full citation record

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