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RS CV sub n binary systemsAn attempt is made to place in context the vast amount of data obtained as a result of X-ray, ultraviolet, optical, and microwave observations of RS CVn and similar spectroscopic binary systems. Emphasis is on the RS CVn systems and their long period analogs. The following questions are considered: (1) are the original defining characteristics still valid and still adequate? (2) what is the evidence for discrete active regions? (3) have any meaningful physical properties for the atmospheres of RS CVn systems been derived? (4) what do the flare observations tell about magnetic fields in RS CVn systems? (5) is there evidence for systematic trends in RS CVn systems with spectral type?
Document ID
19850005395
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Linsky, J. L. (Joint Inst. for Lab. Astrophysics Boulder, CO, United States)
Date Acquired
September 5, 2013
Publication Date
January 1, 1984
Subject Category
Astronomy
Report/Patent Number
NASA-CR-174164
NAS 1.26:174164
Accession Number
85N13704
Funding Number(s)
CONTRACT_GRANT: NGL-06-003-057
CONTRACT_GRANT: NAG5-82
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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