Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares

Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares

CTA 102 is a blazar implying that its relativistic jet points towards Earth and emits synchrotron radiation produced by energetic particles gyrating in the magnetic field. This study aims to figure out the physical origins of radio flares in the jet, including the connection between the magnetic fie...

Full description

Saved in:
Bibliographic Details
Main Authors: Kim, Sang-Hyun, Lee, Sang-Sung, Lee, Jee Won, Hodgson, Jeffrey A., Kang, Sincheol, Algaba Marcos, Juan-Carlos, Kim, Jae-Young, Hodges, Mark, Agudo, Ivan, Fuentes, Antonio, Escudero, Juan, Myserlis, Ioannis, Traianou, Efthalia, Lahteenmaki, Anne, Tornikoski, Merja, Tammi, Joni, Ramakrishnan, Venkatessh, Jarvela, Emilia
Format: Article
Published: Oxford University Press 2022
Subjects:
QB Astronomy
Online Access:http://eprints.um.edu.my/33635/
Tags: Add Tag
No Tags, Be the first to tag this record!
Institution: Universiti Malaya

Internet

http://eprints.um.edu.my/33635/

Similar Items