High-resolution studies of extreme-ultraviolet emission from CO by electron impact

1997 ◽  
Vol 55 (5) ◽  
pp. 3547-3556 ◽  
Author(s):  
Marco Ciocca ◽  
Isik Kanik ◽  
Joseph M. Ajello
1996 ◽  
Vol 152 ◽  
pp. 309-316
Author(s):  
Frits Paerels ◽  
Min Young Hur ◽  
Christopher W. Mauche

A longstanding problem in the interpretation of the X-ray and extreme ultraviolet emission from strongly magnetic cataclysmic variables can be addressed definitively with high resolution EUV spectroscopy. A detailed photospheric spectrum of the accretion-heated polar cap of the white dwarf is sensitive in principle to the temperature structure of the atmosphere. This may allow us to determine where and how the bulk of the accretion energy is thermalized. The EUVE data on AM Herculis and EF Eridani are presented and discussed in this context.


1995 ◽  
Vol 101 ◽  
pp. 375 ◽  
Author(s):  
Xianming Liu ◽  
Syed M. Ahmed ◽  
Rosalie A. Multari ◽  
Geoffrey K. James ◽  
Joseph M. Ajello

1995 ◽  
Vol 51 (3) ◽  
pp. 2067-2074 ◽  
Author(s):  
Isik Kanik ◽  
Geoffrey K. James ◽  
Joseph M. Ajello

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