Formation of resonance spectral line profiles in stellar wind: Theory and observations

1999 ◽  
Vol 18 (3) ◽  
pp. 475-485
Author(s):  
A. Sapar ◽  
L. Sapar
1994 ◽  
Vol 162 ◽  
pp. 534-535
Author(s):  
L. Sapar ◽  
A. Sapar

The resonance spectral lines of high-resolution IUE spectra of χ2 Ori (B2I) have been studied with the aim to determine in more detail the physical status of the stellar wind and its variability due to shell outbursts and clumps superimposed on the isotropic stellar wind. Some general features of resonance spectral line profiles have been studied and explained in physical terms using χ2 Ori as a specimen.


Optik ◽  
2020 ◽  
Vol 202 ◽  
pp. 163485
Author(s):  
Y. Ben Nana ◽  
F. Khelfaoui ◽  
M.T. Meftah ◽  
E. Sadeghzadeh Lari
Keyword(s):  

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