Numerical Simulation of Line Profile Variation in roAp Stars

2009 ◽  
Author(s):  
T. Nomura ◽  
H. Shibahashi ◽  
Joyce Ann Guzik ◽  
Paul A. Bradley
1984 ◽  
Vol 283 ◽  
pp. 218 ◽  
Author(s):  
C. A. Grady ◽  
T. P. Snow ◽  
W. C. Cash

1994 ◽  
Vol 162 ◽  
pp. 368-369
Author(s):  
E. Kambe

We have found that the range in wavelength of the line-profile variations (lpv) in the Be star λ Eridani increases by some 20% during its emission phases. This growth is associated with a possible increase in the equatorial velocity of the star during emission. We discuss the significance of this in connection with other features of the lpv and our earlier discovery of a weak correlation between the amplitude of the lpv and Be outbursts in ζ Ophiuchi.


2008 ◽  
Vol 60 (1) ◽  
pp. 63-76 ◽  
Author(s):  
Hiromoto Shibahashi ◽  
Douglas Gough ◽  
Donald W. Kurtz ◽  
Eiji Kambe

Solar Physics ◽  
1978 ◽  
Vol 60 (2) ◽  
pp. 265-267
Author(s):  
Marc S. Allen

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