Using synchrotron emission modelling of relativistic hydrodynamic jet simulations to study the FR I/FR II dichotomy of active galactic nuclei radio jets-Reference-Cited by-同舟云学术

Using synchrotron emission modelling of relativistic hydrodynamic jet simulations to study the FR I/FR II dichotomy of active galactic nuclei radio jets

Published:2019-03-14 Issue:4 Volume:485 Page:4658-4666
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

van der Westhuizen I P¹,van Soelen B¹^ORCID,Meintjes P J¹,Beall J H²³

Affiliation:

1. Department of Physics, University of the Free State, 205 Nelson Mandela Drive, Bloemfontein 9301, South Africa

2. St. John’s College, 60 College avenue, Annapolis, 21401, USA

3. Space Sciences Division, Naval Research Laboratory, Washington, DC, 20375, USA

Funder

National Research Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/485/4/4658/28227928/stz734.pdf

Reference36 articles.

1. Radio Emission from Three-dimensional Relativistic Hydrodynamic Jets: Observational Evidence of Jet Stratification

2. Pilot study of the radio-emitting AGN population: the emerging new class of FR 0 radio-galaxies

3. The accretion mechanism in low-power radio galaxies

4. Revised equipartition and minimum energy formula for magnetic field strength estimates from radio synchrotron observations

5. A 'Twin-Exhaust' Model for Double Radio Sources

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