Distribution of Faraday Rotation Measure in Jets from Active Galactic Nuclei. II. Prediction from Our Sweeping Magnetic Twist Model for the Wiggled Parts of Active Galactic Nucleus Jets and Tails

2004 ◽  
Vol 608 (1) ◽  
pp. 119-135 ◽  
Author(s):  
Hiromitsu Kigure ◽  
Yutaka Uchida ◽  
Masanori Nakamura ◽  
Shigenobu Hirose ◽  
Robert Cameron
Galaxies ◽  
2018 ◽  
Vol 6 (2) ◽  
pp. 40
Author(s):  
Alice Pasetto ◽  
Carlos Carrasco-González ◽  
Shane O’Sullivan ◽  
Aritra Basu ◽  
Gabriele Bruni ◽  
...  

2004 ◽  
Vol 600 (1) ◽  
pp. 88-95 ◽  
Author(s):  
Yutaka Uchida ◽  
Hiromitsu Kigure ◽  
Shigenobu Hirose ◽  
Masanori Nakamura ◽  
Robert Cameron

2017 ◽  
Vol 472 (2) ◽  
pp. 1792-1801 ◽  
Author(s):  
D. C. Gabuzda ◽  
N. Roche ◽  
A. Kirwan ◽  
S. Knuettel ◽  
M. Nagle ◽  
...  

2012 ◽  
Vol 144 (4) ◽  
pp. 105 ◽  
Author(s):  
Talvikki Hovatta ◽  
Matthew L. Lister ◽  
Margo F. Aller ◽  
Hugh D. Aller ◽  
Daniel C. Homan ◽  
...  

2013 ◽  
Vol 9 (S303) ◽  
pp. 54-58
Author(s):  
Deokkeun An ◽  
Solange V. Ramírez ◽  
Kris Sellgren

AbstractWe present 10 μm – 35μm Spitzer spectra of the interstellar medium in the central molecular zone (CMZ), the central 210 pc × 60 pc of the Galactic center (GC). We present maps of the CMZ in ionic and H2 emission, covering a more extensive area than earlier spectroscopic surveys in this region. We compare diagnostic line ratios measured in the Spitzer Infrared Nearby Galaxies Survey to our data. Previous work shows that forbidden line ratios can distinguish star-forming galaxies from low-ionization nuclear emission-line regions (LINERs) and active galactic nuclei (AGNs). Our GC line ratios agree with star-forming galaxies and not with LINERs or AGNs.


Sign in / Sign up

Export Citation Format

Share Document