[ITAL]Chandra[/ITAL] Observations of the X-Ray Narrow-Line Region in NGC 4151

2000 ◽  
Vol 545 (2) ◽  
pp. L81-L84 ◽  
Author(s):  
P. M. Ogle ◽  
H. L Marshall ◽  
J. C. Lee ◽  
C. R. Canizares
1989 ◽  
Vol 134 ◽  
pp. 352-354
Author(s):  
Hartmut Schulz ◽  
Berto Boer

Line profiles from the spatially resolved narrow-line region of NGC 4151 are separated into several bulk-motion components which show velocity dispersions two to three times larger than starburst nuclei with similar luminosity. The components are suggested to arise within the galactic disk and by filaments entrained in or situated along the shells of two super-bubbles. The large cone-like SW bubble is able to account for the SW soft-X ray excess and the hole in the NLR disk through which a UV-radiation cone emerges. The bubbles appear to be related to the nuclear radio source.


1999 ◽  
Vol 118 (5) ◽  
pp. 2101-2107 ◽  
Author(s):  
J. B. Hutchings ◽  
D. M. Crenshaw ◽  
A. C. Danks ◽  
T. R. Gull ◽  
S. B. Kraemer ◽  
...  

2003 ◽  
Vol 126 (3) ◽  
pp. 1167-1182 ◽  
Author(s):  
Tohru Nagao ◽  
Takashi Murayama ◽  
Yasuhiro Shioya ◽  
Yoshiaki Taniguchi

2008 ◽  
Vol 679 (2) ◽  
pp. 1128-1143 ◽  
Author(s):  
S. B. Kraemer ◽  
H. R. Schmitt ◽  
D. M. Crenshaw

2000 ◽  
Vol 531 (1) ◽  
pp. 278-295 ◽  
Author(s):  
S. B. Kraemer ◽  
D. M. Crenshaw ◽  
J. B. Hutchings ◽  
T. R. Gull ◽  
M. E. Kaiser ◽  
...  

1998 ◽  
Vol 188 ◽  
pp. 436-437
Author(s):  
C. Otani ◽  
T. Kii ◽  
K. Miya

We report the results of the search for the change in the warm absorber of the quasar MR 2251-178 with ASCA. We detected its change along with the X-ray intensity change. In the bright phase in 1993, its X-ray spectra showed the absorption edge features by OVII and OVIII edges. In contrast, in the medium intensity (in 1996), the absorption apparently increased and the edge energy was shifted to the lower energy. These results are well explained by the ionization change of the same absorber. The timescale of the change requires moderately high density and the location to be nearer to the center than the Narrow Line Region. We briefly discuss the stability of the warm absorber.


Author(s):  
M. E. Kaiser ◽  
L. D. Bradley ◽  
J. B. Hutchings ◽  
D. M. Crenshaw ◽  
S. B. Kraemer ◽  
...  

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