Detection of a Violent Line Profile Variation of the [TSUP]28[/TSUP]S[CLC]i[/CLC]O [CLC][ITAL]v[/ITAL][/CLC] = 2, [ITAL]J[/ITAL] = 3–2 Maser Emission toward Orion KL IR[CLC]c[/CLC]2

1999 ◽  
Vol 117 (3) ◽  
pp. 1485-1489 ◽  
Author(s):  
Se-Hyung Cho ◽  
Hyun-Soo Chung ◽  
Hyo-Ryoung Kim ◽  
Hyun-Goo Kim ◽  
Duk-Gyoo Roh
Keyword(s):  
Line Profile ◽  
Maser Emission ◽  
Profile Variation ◽  
Line Profile Variation

Numerical Simulation of Line Profile Variation in roAp Stars

2009 ◽  
Author(s):  
T. Nomura ◽  
H. Shibahashi ◽  
Joyce Ann Guzik ◽  
Paul A. Bradley
Keyword(s):  
Numerical Simulation ◽  
Line Profile ◽  
Profile Variation ◽  
Line Profile Variation

Line profile variation in delta-Orionis A, l-Orionis A, and 15 Monocerotis

1984 ◽  
Vol 283 ◽  
pp. 218 ◽  
Author(s):  
C. A. Grady ◽  
T. P. Snow ◽  
W. C. Cash
Keyword(s):  
Line Profile ◽  
Profile Variation ◽  
Line Profile Variation

scholarly journals Growth of the line-profile variation region during Be episodes

1994 ◽  
Vol 162 ◽  
pp. 368-369
Author(s):  
E. Kambe
Keyword(s):  
Line Profile ◽  
Weak Correlation ◽  
Profile Variation ◽  
Be Star ◽  
Line Profile Variation

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.

scholarly journals Shock Waves and Line-Profile Variation in roAp Stars

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

Supergranular line profile variation of Mg i ?2852

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