The Composition and Power of the Jet of the Broad-line Radio Galaxy 3C 120
We calculated the electron-positron pair-production rate at the base of the jet of 3C 120 due to collisions of photons from the hot accretion flow using the measurement of its average soft gamma-ray spectrum by the Compton Gamma Ray Observatory. We found that this rate approximately equals the flow...
Main Authors: | Böttcher, M. (Author), Chibueze, J.O (Author), Phuravhathu, D.G (Author), Sikora, M. (Author), Zdziarski, A.A (Author) |
---|---|
Format: | Article |
Language: | English |
Published: |
American Astronomical Society
2022
|
Online Access: | View Fulltext in Publisher |
Similar Items
-
The jets in radio galaxies
by: Hardcastle, M. J.
Published: (1997) -
The Connection between the Radio Jet and the γ-ray Emission in the Radio Galaxy 3C 120 and the Blazar CTA 102
by: Carolina Casadio, et al.
Published: (2016-09-01) -
Jet-cloud interactions in powerful radio galaxies
by: Clark, Neil Edward
Published: (1996) -
The Connection between the Radio Jet and the γ-ray Emission in the Radio Galaxy 3C 120 and the Blazar CTA 102
by: Casadio, Carolina, et al.
Published: (2016) -
JET-POWERED MOLECULAR HYDROGEN EMISSION FROM RADIO GALAXIES
by: Ogle, Patrick M., et al.
Published: (2015)