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...

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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
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Published: Oxford University Press 2022
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Online Access:http://eprints.um.edu.my/33635/
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spelling my.um.eprints.336352022-07-28T01:12:00Z http://eprints.um.edu.my/33635/ Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares 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 QB Astronomy 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 field and the radio flares. The data set in the range of 2.6-343.5 GHz was collected over a period of similar to 5.5 yr (2012 November 20-2018 September 23). During the data collection period, seven flares at 15 GHz with a range of the variability time-scale of roughly 76-227 d were detected. The quasi-simultaneous radio data were used to investigate the synchrotron spectrum of the source. We found that the synchrotron radiation is self-absorbed. The turnover frequency and the peak flux density of the synchrotron self-absorption (SSA) spectra are in the ranges of similar to 42-172 GHz and similar to 0.9-10.2 Jy, respectively. From the SSA spectra, we derived the SSA magnetic field strengths to be similar to 9.20, similar to 12.28, and similar to 50.97 mG on 2013 December 24, 2014 February 28, and 2018 January 13, respectively. We also derived the equipartition magnetic field strengths to be in the range of similar to 24-109 mG. The equipartition magnetic field strengths are larger than the SSA magnetic field strengths in most cases, which indicates that particle energy mainly dominates in the jet. Our results suggest that the flares in the jet of CTA 102 originated due to particle acceleration. We propose the possible mechanisms of particle acceleration. Oxford University Press 2022-02 Article PeerReviewed Kim, Sang-Hyun and Lee, Sang-Sung and Lee, Jee Won and Hodgson, Jeffrey A. and Kang, Sincheol and Algaba Marcos, Juan-Carlos and Kim, Jae-Young and Hodges, Mark and Agudo, Ivan and Fuentes, Antonio and Escudero, Juan and Myserlis, Ioannis and Traianou, Efthalia and Lahteenmaki, Anne and Tornikoski, Merja and Tammi, Joni and Ramakrishnan, Venkatessh and Jarvela, Emilia (2022) Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares. Monthly Notices of the Royal Astronomical Society, 510 (1). pp. 815-833. ISSN 0035-8711, DOI https://doi.org/10.1093/mnras/stab3473 <https://doi.org/10.1093/mnras/stab3473>. 10.1093/mnras/stab3473
institution Universiti Malaya
building UM Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider Universiti Malaya
content_source UM Research Repository
url_provider http://eprints.um.edu.my/
topic QB Astronomy
spellingShingle QB Astronomy
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
Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares
description 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 field and the radio flares. The data set in the range of 2.6-343.5 GHz was collected over a period of similar to 5.5 yr (2012 November 20-2018 September 23). During the data collection period, seven flares at 15 GHz with a range of the variability time-scale of roughly 76-227 d were detected. The quasi-simultaneous radio data were used to investigate the synchrotron spectrum of the source. We found that the synchrotron radiation is self-absorbed. The turnover frequency and the peak flux density of the synchrotron self-absorption (SSA) spectra are in the ranges of similar to 42-172 GHz and similar to 0.9-10.2 Jy, respectively. From the SSA spectra, we derived the SSA magnetic field strengths to be similar to 9.20, similar to 12.28, and similar to 50.97 mG on 2013 December 24, 2014 February 28, and 2018 January 13, respectively. We also derived the equipartition magnetic field strengths to be in the range of similar to 24-109 mG. The equipartition magnetic field strengths are larger than the SSA magnetic field strengths in most cases, which indicates that particle energy mainly dominates in the jet. Our results suggest that the flares in the jet of CTA 102 originated due to particle acceleration. We propose the possible mechanisms of particle acceleration.
format Article
author 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
author_facet 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
author_sort Kim, Sang-Hyun
title Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares
title_short Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares
title_full Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares
title_fullStr Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares
title_full_unstemmed Magnetic field strengths of the synchrotron self-absorption region in the jet of CTA 102 during radio flares
title_sort magnetic field strengths of the synchrotron self-absorption region in the jet of cta 102 during radio flares
publisher Oxford University Press
publishDate 2022
url http://eprints.um.edu.my/33635/
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score 13.15806