scholarly journals Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from theHubble Space Telescope

1999 ◽  
Vol 516 (2) ◽  
pp. 750-768 ◽  
Author(s):  
D. Michael Crenshaw ◽  
Steven B. Kraemer ◽  
Albert Boggess ◽  
Stephen P. Maran ◽  
Richard F. Mushotzky ◽  
...  
2001 ◽  
Vol 557 (1) ◽  
pp. 2-17 ◽  
Author(s):  
M. J. Collinge ◽  
W. N. Brandt ◽  
Shai Kaspi ◽  
D. Michael Crenshaw ◽  
Martin Elvis ◽  
...  

1986 ◽  
Vol 119 ◽  
pp. 575-576
Author(s):  
P M Gondhalekar ◽  
N Brosch

Absorption lines at the redshifts of cosmic voids in Perseus-Pisces and Böotes have been detected in the ultraviolet spectra of background quasars. The detection of Si IV and C IV lines besides Ly α suggests chemical enrichment of gas in the voids. Additional observations of three sight-lines through the void in the Böotes suggests that the gas in the void is clumped in large clouds.


2014 ◽  
Vol 792 (1) ◽  
pp. 77 ◽  
Author(s):  
Toru Misawa ◽  
Jane C. Charlton ◽  
Michael Eracleous

2004 ◽  
Vol 601 (2) ◽  
pp. 715-722 ◽  
Author(s):  
Desika Narayanan ◽  
Fred Hamann ◽  
Tom Barlow ◽  
E. M. Burbidge ◽  
Ross D. Cohen ◽  
...  

2013 ◽  
Vol 435 (2) ◽  
pp. 1233-1264 ◽  
Author(s):  
Rajib Ganguly ◽  
Ryan S. Lynch ◽  
Jane C. Charlton ◽  
Michael Eracleous ◽  
Todd M. Tripp ◽  
...  

1997 ◽  
Vol 478 (1) ◽  
pp. 80-86 ◽  
Author(s):  
Fred Hamann ◽  
Thomas A. Barlow ◽  
Vesa Junkkarinen ◽  
E. M. Burbidge

1997 ◽  
Vol 159 ◽  
pp. 240-243 ◽  
Author(s):  
D.M. Crenshaw

AbstractRecentHSTspectra indicate that a large fraction of Seyfert 1 galaxies have UV absorption lines that are intrinsic to the active nucleus or its environment.IUEmonitoring or multipleHSTobservations of several sources show that many absorption lines are variable, either as a result of mass motion across the line-of-sight or of changing ionization within the gas in response to variations in the ionizing continuum. The UV absorbers may be related to the warm absorbers seen in the X-ray spectra of many Seyfert galaxies, but a direct connection between the two has not been made. Some of the absorption lines may arise in the emission-line regions in the nucleus or host galaxy, providing valuable clues to their nature.


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