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IUE spectra of a flare in HR 5110: A flaring RS CVn or Algol system?Ultraviolet spectra of the RS CVn type binary system HR 5110 were obtained with IUE on May 31, 1979 during a period of intense radio flaring of this star. High temperature transition region lines are present, but are not enhanced above observed quiescent strengths. The similarities of HR 5110 to the Algol system, As Eri, suggest that the 1979 May to June flare may involve mass exchange rather than annihilation of coronal magnetic fields.
Document ID
19810017402
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Simon, T. (Joint Inst. for Lab. Astrophysics Boulder, CO, United States)
Linsky, J. L. (Joint Inst. for Lab. Astrophysics Boulder, CO, United States)
Schiffer, F. H., III (Computer Sciences Corp.)
Date Acquired
August 11, 2013
Publication Date
January 1, 1981
Publication Information
Publication: NASA. Goddard Space Flight Center The Universe at Ultraviolet Wavelengths: The First Two Yrs. of Intern. Ultraviolet Explorer
Subject Category
Astrophysics
Accession Number
81N25938
Funding Number(s)
CONTRACT_GRANT: NAS5-23274
CONTRACT_GRANT: NGL-06-003-057
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19810017357Collected WorksThe Universe at Ultraviolet Wavelengths: The first two years of International Ultraviolet Explorer19810017357Collected WorksThe Universe at Ultraviolet Wavelengths: The first two years of International Ultraviolet Explorer
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