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Cool magnetic CP starsThe paper reviews progress in research on the cool magnetic CP stars especially during the past four years. Studies of energy distributions and abundances are analyzed to reveal their systematics. Model atmospheres do not yet accurately describe the average energy distributions much less the variability with the rotational periods of these stars.
Document ID
19870043087
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Adelman, Saul J. (NASA Goddard Space Flight Center Greenbelt, MA, United States)
Cowley, Charles R. (Michigan, University Ann Arbor, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1986
Subject Category
Astrophysics
Accession Number
87A30361
Distribution Limits
Public
Copyright
Other

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