Transfer of line radiation in differentially expanding atmospheres. V - Line formation in a decelerating spherical flow

1977 ◽  
Vol 215 ◽  
pp. 247 ◽  
Author(s):  
F. Marti ◽  
P. D. Noerdlinger
1972 ◽  
Vol 25 (2) ◽  
pp. 177 ◽  
Author(s):  
CJ Cannon

The multidimensional equation of transfer for spectral line radiation under a general redistribution law is studied. It is shown that the equation may be rewritten as a system of equations of the "Feautrier" form, which are known to be exceedingly stable and efficient under numerical reduction. It is also shown that the inclusion of a multidimensional differential macroscopic velocity field does not alter the functional form of the equations obtained and therefore may also be treated by the general Feautrier technique.


1976 ◽  
Vol 70 ◽  
pp. 281-312
Author(s):  
D. G. Hummer

The current state of understanding of line formation processes in expanding atmospheres is reviewed, and the successes and limitations of current computational techniques are summarized. Some results for differential rotation are also given, although very little work has been done in this area. Special attention is given to the severe difficulties that are encountered in inferring the structure of rapidly expanding or rotating atmospheres from observed line profiles because of the failure under these conditions of the Eddington-Barbier relation in integrated light; the value in this respect of continuum and interferometric observations is emphasized.


1974 ◽  
Vol 193 ◽  
pp. 651 ◽  
Author(s):  
P. D. Noerdlinger ◽  
G. B. Rybicki

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