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EUV spectroscopy of 3 RSCVn binariesThe extreme ultraviolet (EUV) spectroscopy of several binary stars containing cool components is used to define the high temperature plasma structure of these stars and their stellar atmospheres. Different line emission spectra are reported, along with a spectrum analysis of Capella, a nearby bright multiple star system, using data from the EUVE satellite.
Document ID
19960007141
Acquisition Source
Legacy CDMS
Document Type
Preprint (Draft being sent to journal)
Authors
Dupree, A. K. (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Brickhouse, Nancy S. (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Hanson, G. J. (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Date Acquired
September 6, 2013
Publication Date
August 1, 1995
Subject Category
Astrophysics
Report/Patent Number
PREPRINT-4119
NIPS-95-05607
Accession Number
96N14306
Funding Number(s)
CONTRACT_GRANT: NAG5-2330
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19960007142WorkHigh temperature structure in cool binary stars19960007143WorkDissecting the EUV spectrum of Capella
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