Variability of the Broad Emission Line Profiles in NGC 5548

1992 ◽  
pp. 200-201
Author(s):  
Matthias Dietrich ◽  
Wolfram Kollatschny
1997 ◽  
Vol 159 ◽  
pp. 193-194 ◽  
Author(s):  
C. Martin Gaskell ◽  
Stephanie A. Snedden

AbstractWe postulate that all structure in broad lines can be explained by a central component (at the systemic redshift) and the addition of two ‘displaced components’, one blueshifted and the other redshifted. We have been able to successfully classify all Balmer-line profiles on this basis. 3C 390.3-type objects are merely examples where the shifts of the displaced components are unusually large. We believe that the displaced peaks are less prominent in the UV lines because the higher ionization lines are broader.


1997 ◽  
Vol 479 (1) ◽  
pp. 200-221 ◽  
Author(s):  
Mark Bottorff ◽  
Kirk T. Korista ◽  
Isaac Shlosman ◽  
Roger D. Blandford

1996 ◽  
Vol 463 ◽  
pp. 144 ◽  
Author(s):  
Christine Done ◽  
Julian H. Krolik

1997 ◽  
Vol 159 ◽  
pp. 197-198
Author(s):  
Giovanna M. Stirpe ◽  
Andrew Robinson ◽  
David J. Axon

AbstractWe present preliminary results from a study of broad-line profiles in active galaxies. A simple model in which the emissivity is a broken power-law function of radius, and the BLR clouds emit anisotropically, yields very good fits to almost all the Ha profiles in our data base.


2009 ◽  
Vol 53 (7-10) ◽  
pp. 191-197 ◽  
Author(s):  
A.I. Shapovalova ◽  
L.Č. Popović ◽  
N.G. Bochkarev ◽  
A.N. Burenkov ◽  
V.H. Chavushyan ◽  
...  

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