IUE observations of NGC 5548, 1978-1988 - The sizes and kinematics of the broad-line region

1991 ◽  
Vol 375 ◽  
pp. 85 ◽  
Author(s):  
Anuradha P. Koratkar ◽  
C. M. Gaskell
1998 ◽  
Vol 184 ◽  
pp. 467-468
Author(s):  
N.G. Bochkarev ◽  
A.I. Shapovalova ◽  
A.N. Burenkov ◽  
V.V. Vlasyuk

To study broad line region (BLR) size and kinematics spectral monitoring of NGC 3516, NGC 4151, NGC 5548, NGC 7469 and 3C390.3 has been performed with the 6 m telescope of the Special Astrophysical Observatory (N. Arkhyz- North Caucasus) in 1986–1996. The spectra are obtained in the Nasmyth focus using the TV scanner with a resolution of 3–4Å and S/N= 10–25 within 4000–5200ÅÅ (1986–94, 500 spectra), and in the prime focus with the spectrograph UAGS (a long-slit mode) + CCD (resolution 5–10Å) or multi-pupil field spectrograph (MPFS) + CCD (resolution 4Å) within 4000–7000ÅÅ and S/N=50–100 (1995–96, 270 spectra).


2016 ◽  
Vol 827 (2) ◽  
pp. 118 ◽  
Author(s):  
Kai-Xing Lu ◽  
Pu Du ◽  
Chen Hu ◽  
Yan-Rong Li ◽  
Zhi-Xiang Zhang ◽  
...  

1991 ◽  
Vol 371 ◽  
pp. 541 ◽  
Author(s):  
J. H. Krolik ◽  
Keith Horne ◽  
T. R. Kallman ◽  
M. A. Malkan ◽  
R. A. Edelson ◽  
...  

1997 ◽  
Vol 159 ◽  
pp. 215-216 ◽  
Author(s):  
M.C. Bottorff ◽  
K.T. Korista ◽  
I. Shlosman ◽  
R.D. Blandford

AbstractA hydromagnetic wind model from a dusty molecular disk (Emmering, Blandford, & Shlosman 1992) was applied to the BLR in NGC 5548 and produced synthetic C IV line profiles as a function of time. The model C IV profiles are compared to data from the 1993 IUE/HST campaign and properties of the the BLR of NGC 5548 are inferred.


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