scholarly journals Space Telescope and Optical Reverberation Mapping Project. IX. Velocity–Delay Maps for Broad Emission Lines in NGC 5548

2021 ◽  
Vol 907 (2) ◽  
pp. 76
Author(s):  
Keith Horne ◽  
G. De Rosa ◽  
B. M. Peterson ◽  
A. J. Barth ◽  
J. Ely ◽  
...  
2020 ◽  
Vol 898 (2) ◽  
pp. 141 ◽  
Author(s):  
M. Dehghanian ◽  
G. J. Ferland ◽  
G. A. Kriss ◽  
B. M. Peterson ◽  
K. T. Korista ◽  
...  

2017 ◽  
Vol 846 (1) ◽  
pp. 55 ◽  
Author(s):  
S. Mathur ◽  
A. Gupta ◽  
K. Page ◽  
R. W. Pogge ◽  
Y. Krongold ◽  
...  

2017 ◽  
Vol 835 (1) ◽  
pp. 65 ◽  
Author(s):  
D. Starkey ◽  
Keith Horne ◽  
M. M. Fausnaugh ◽  
B. M. Peterson ◽  
M. C. Bentz ◽  
...  

2004 ◽  
Vol 422 (3) ◽  
pp. 925-940 ◽  
Author(s):  
A. I. Shapovalova ◽  
V. T. Doroshenko ◽  
N. G. Bochkarev ◽  
A. N. Burenkov ◽  
L. Carrasco ◽  
...  

Author(s):  
A.I. SHAPOVALOVA ◽  
V.T. DOROSHENKO ◽  
N.G. BOCHKAREV ◽  
A.N. BURENKOV ◽  
L. CARRASCO ◽  
...  

2016 ◽  
Vol 821 (1) ◽  
pp. 56 ◽  
Author(s):  
M. M. Fausnaugh ◽  
K. D. Denney ◽  
A. J. Barth ◽  
M. C. Bentz ◽  
M. C. Bottorff ◽  
...  

2014 ◽  
Vol 10 (S313) ◽  
pp. 43-47 ◽  
Author(s):  
J. León Tavares ◽  
V. Chavushyan ◽  
A. Lobanov ◽  
E. Valtaoja ◽  
T. G. Arshakian

AbstractAGN reverberate when the broad emission lines respond to changes of the ionizing thermal continuum emission. Reverberation measurements have been commonly used to estimate the size of the broad-line region (BLR) and the mass of the central black hole. However, reverberation mapping studies have been mostly performed on radio-quiet sources where the contribution of the jet can be neglected. In radio-loud AGN, jets and outflows may affect substantially the relation observed between the ionizing continuum and the line emission. To investigate this relation, we have conducted a series of multi-wavelength studies of radio-loud AGN, combining optical spectral line monitoring with regular VLBI observations. Our results suggest that at least a fraction of the broad-line emitting material can be located in a sub-relativistic outflow ionized by non-thermal continuum emission generated in the jet at large distances (> 1 pc) from the central engine of AGN. This finding may have a strong impact on black hole mass estimates based on measured widths of the broad emission lines and on the gamma-ray emission mechanisms.


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