Fermi Large Area Telescope detection of bright γ-ray outbursts from the peculiar quasar 4C +21.35
Journal Article
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· The Astrophysical Journal
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- Institute of Space and Astronautical Science, Kanagawa (Japan)
- Institute of Space and Astronautical Science, Kanagawa (Japan); Jagiellonian Univ., Krakow (Poland)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- IASF Palermo, Palermo (Italy); INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica, Roma (Italy)
- Ecole Polytechnique, Palaiseau (France)
- Univ. Bordeaux, Gradignan (France)
- Naval Research Lab., Washington, D.C. (United States)
- National Academy of Science, Washington, D.C. (United States); Naval Research Lab., Washington, D.C. (United States)
- Istituto Nazionale di Fisica Nucleare, Padova (Italy); Univ. di Padova, Padova (Italy)
- Univ. Bordeaux, Gradignan (France); Centre d'Etudes Nucleaires Bordeaux Gradignan, Gradignan (France)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States); Univ. of Maryland, College Park, MD (United States)
- Stanford Univ., Stanford, CA (United States)
- INAF Istituto di Radioastronomia, Bologna (Italy)
- Max-Planck-Institut fur Radioastronomie, Bonn (Germany)
- Istituto Nazionale di Fisica Nucleare, Trieste (Italy); Osservatorio Astronomico di Trieste, Trieste (Italy)
- Univ. degli Studi di Perugia, Perugia (Italy)
In this study, we report on the two-year-long Fermi-Large Area Telescope observation of the peculiar blazar 4C +21.35 (PKS 1222+216). This source was in a quiescent state from the start of the science operations of the Fermi Gamma-ray Space Telescope in 2008 August until 2009 September, and then became more active, with gradually increasing flux and some moderately bright flares. In 2010 April and June, 4C +21.35 underwent a very strong GeV outburst composed of several major flares characterized by rise and decay timescales of the order of a day. During the outburst, the GeV spectra of 4C +21.35 displayed a broken power-law form with spectral breaks observed near 1-3 GeV photon energies. We demonstrate that, at least during the major flares, the jet in 4C +21.35 carried a total kinetic luminosity comparable to the total accretion power available to feed the outflow. We also discuss the origin of the break observed in the flaring spectra of 4C +21.35. We show that, in principle, a model involving annihilation of the GeV photons on the He II Lyman recombination continuum and line emission of "broad-line region" clouds may account for such. However, we also discuss the additional constraint provided by the detection of 4C +21.35 at 0.07-0.4 TeV energies by the MAGIC telescope, which coincided with one of the GeV flares of the source. We argue that there are reasons to believe that the lesssim TeV emission of 4C +21.35 (as well as the GeV emission of the source, if co-spatial) is not likely to be produced inside the broad-line region zone of highest ionization (~1017 cm from the nucleus), but instead originates further away from the active center, namely, around the characteristic scale of the hot dusty torus surrounding the 4C +21.35 nucleus (~1019 cm).
- Research Organization:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC02-76SF00515
- OSTI ID:
- 1357257
- Alternate ID(s):
- OSTI ID: 21576800
- Journal Information:
- The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 1 Vol. 733; ISSN 0004-637X
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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