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Ne V and Ne VI Lines in the Ultraviolet Spectrum of the Symbiotic Star RR Telescopii
 

Summary: Ne V and Ne VI Lines in the Ultraviolet Spectrum of the
Symbiotic Star RR Telescopii
B. Espey 1;2
Center for Astrophysical Sciences, Department of Physics and Astronomy,
The Johns Hopkins University, Baltimore MD 21218; espey@pha.jhu.edu
F. P. Keenan and F. C. McKenna
Department of Pure and Applied Physics, The Queen's University of Belfast,
Belfast BT7 1NN, Northern Ireland, UK; f.keenan@qub.ac.uk; f.mckenna@qub.ac.uk
W. A. Feibelman 3
Laboratory for Astronomy and Solar Physics, Code 684.1, NASA--Goddard Space Flight
Center, Greenbelt MD 20771; feibelman@iue.gsfc.nasa.gov
and
K. M. Aggarwal
Department of Physics and Astrophysics, University of Delhi, Delhi 110 007, India
Received October 11 1995; accepted January 2 1996
accepted by the Astrophysical Journal, main journal
1 also Department of Physics & Astronomy, University of Pittsburgh, Pittsburgh,
PA 15260
2 Guest Investigator, Astro­2 mission
3 Guest observer with the International Ultraviolet Explorer satellite, which is operated

  

Source: Henry, Richard C.- Department of Physics and Astronomy, Johns Hopkins University

 

Collections: Physics