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Discrepant asymmetry stars: The role of unsteady magnetic flux loops in the atmospheres of late-type giant starsA number of spectroscopic peculiarities of K giants and other stars which lie in a wedge in the HR diagram are discussed. These peculiarities can be understood in terms of unsteady magnetic flux loops emerging into the stellar atmosphere from beneath the surface.
Document ID
19820023318
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Mullan, D. J.
(Delaware Univ. Newark, DE, United States)
Stencel, R. E.
(Joint Inst. for Lab. Astrophysics)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Publication Information
Publication: NASA. Goddard Space Flight Center Advan. in Ultraviolet Astron.
Subject Category
Astronomy
Accession Number
82N31194
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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