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Title: A combined radio and GeV γ-ray view of the 2012 and 2013 flares of Mrk 421

Journal Article · · Monthly Notices of the Royal Astronomical Society
DOI:https://doi.org/10.1093/mnras/stv220· OSTI ID:1355165
 [1];  [2];  [2];  [2];  [3];  [4];  [5];  [6];  [7];  [8];  [4]
  1. Aalto Univ. Metsahovi Radio Observatory, Kylmala (Finland); California Inst. of Technology (CalTech), Pasadena, CA (United States)
  2. Purdue Univ., West Lafayette, IN (United States)
  3. Univ. of Turku, Piikkio (Finland)
  4. California Inst. of Technology (CalTech), Pasadena, CA (United States)
  5. Aalto Univ. Metsahovi Radio Observatory, Kylmala (Finland); Aalto Univ. (Finland). Dept. of Radio Science and Engineering
  6. Univ. Bordeaux, Gradignan (France); CNRS, IN2P3, CENBG, Gradignan (France)
  7. National Radio Astronomy Observatory, Socorro, NM (United States)
  8. Aalto Univ. Metsahovi Radio Observatory, Kylmala (Finland)

In 2012 Markarian 421 underwent the largest flare ever observed in this blazar at radio frequencies. In the present study, we start exploring this unique event and compare it to a less extreme event in 2013. We use 15 GHz radio data obtained with the Owens Valley Radio Observatory 40-m telescope, 95 GHz millimetre data from the Combined Array for Research in Millimeter-Wave Astronomy, and GeV γ-ray data from the Fermi Gamma-ray Space Telescope. Here, the radio light curves during the flaring periods in 2012 and 2013 have very different appearances, in both shape and peak flux density. Assuming that the radio and γ-ray flares are physically connected, we attempt to model the most prominent sub-flares of the 2012 and 2013 activity periods by using the simplest possible theoretical framework. We first fit a one-zone synchrotron self-Compton (SSC) model to the less extreme 2013 flare and estimate parameters describing the emission region. We then model the major γ-ray and radio flares of 2012 using the same framework. The 2012 γ-ray flare shows two distinct spikes of similar amplitude, so we examine scenarios associating the radio flare with each spike in turn. In the first scenario, we cannot explain the sharp radio flare with a simple SSC model, but we can accommodate this by adding plausible time variations to the Doppler beaming factor. In the second scenario, a varying Doppler factor is not needed, but the SSC model parameters require fine-tuning. Both alternatives indicate that the sharp radio flare, if physically connected to the preceding γ-ray flares, can be reproduced only for a very specific choice of parameters.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1355165
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 448, Issue 4; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 38 works
Citation information provided by
Web of Science

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Cited By (19)

Long-term multi-wavelength variability and correlation study of Markarian 421 from 2007 to 2009 journal September 2016
Resolving the High-Energy Universe with Strong Gravitational Lensing: the case of pks 1830–211 journal August 2015
Particle diffusion and localized acceleration in inhomogeneous AGN jets – II. Stochastic variation journal March 2016
The presence of interstellar scintillation in the 15 GHz interday variability of 1158 OVRO-monitored blazars journal September 2019
On the Connection of Radio and γ-Ray Emission in Blazars journal December 2018
X-Ray Flaring Activity of mrk 421 in the First half of 2013 journal October 2016
4.5 Years of Multi-Wavelength Observations of mrk 421 During the Argo-Ybj and Fermi Common Operation time journal January 2016
Swift Observations of Mrk 421 in Selected Epochs. II. An Extreme Spectral Flux Variability in 2009–2012 journal May 2018
3FHL: The Third Catalog of Hard Fermi -LAT Sources journal September 2017
Long-term Optical Polarization Variability and Multiwavelength Analysis of Blazar Mrk 421 journal August 2017
Particle diffusion and localized acceleration in inhomogeneous AGN jets – II. Stochastic variation text January 2016
3FHL: The Third Catalog of Hard Fermi -LAT Sources text January 2017
Long-term multi-wavelength variability and correlation study of Markarian 421 from 2007 to 2009 text January 2016
Resolving the High Energy Universe with Strong Gravitational Lensing: The Case of PKS 1830-211 text January 2015
Long-term multi-wavelength variability and correlation study of Markarian 421 from 2007 to 2009 text January 2016
3FHL: The Third Catalog of Hard Fermi-LAT Sources text January 2017
Long-term optical polarization variability and multiwavelength analysis of Blazar Mrk 421 text January 2017
The presence of interstellar scintillation in the 15 GHz interday variability of 1158 OVRO-monitored blazars text January 2019
Time-dependent neutrino emission from Mrk 421 during flares and predictions for IceCube text January 2016

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