Minute-Timescale >100 MeV gamma-ray variability during the giant outburst of quasar 3C 279 observed by Fermi-LAT in 2015 June

Markus Ackermann R. Anantua K. Asano 1 Luca Baldini Guido Barbiellini D. Bastieri J. Becerra Gonzalez R. Bellazzini E. Bissaldi R. D. Blandford E. D. Bloom R. Bonino E. Bottacini R. Buehler G. A. Caliandro R. A. Cameron M. Caragiulo P. A. Caraveo E. Cavazzuti C. Cecchi 2 C. C. Cheung 3 J. Chiang G. Chiaro S. Ciprini J. Cohen-Tanugi F. Costanza S. Cutini F. D’ammando F. De Palma R. Desiante S. W. Digel 4 N. Di Lalla 5 M. Di Mauro 6 L. Di Venere P. S. Drell C. Favuzzi S. J. Fegan E. C. Ferrara 7 Y. Fukazawa S. Funk 8 P. Fusco 9 F. Gargano D. Gasparrini N. Giglietto F. Giordano M. Giroletti 10 I. A. Grenier 11 Lucas Guillemot 12, 13 S. Guiriec M. Hayashida E. Hays D. Horan 14 G. Jóhannesson S. Kensei D. Kocevski M. Kuss 15 G. La Mura 16 S. Larsson 17 L. Latronico J. Li 18 F. Longo F. Loparco 19 B. Lott 20 M. N. Lovellette P. Lubrano G. M. Madejski J. D. Magill S. Maldera A. Manfreda M. Mayer 21 M. N. Mazziotta P. F. Michelson 22 N. Mirabal T. Mizuno M. E. Monzani A. Morselli I. V. Moskalenko K. Nalewajko M. Negro 23 E. Nuss 19 T. Ohsugi E. Orlando D. Paneque J. S. Perkins 24 M. Pesce-Rollins F. Piron 19 G. Pivato T. A. Porter 25 G. Principe R. Rando M. Razzano S. Razzaque A. Reimer J. D. Scargle C. Sgrò 26 M. Sikora D. Simone 27 E. J. Siskind F. Spada P. Spinelli 28 L. Stawarz J. B. Thayer D. J. Thompson 29 D. F. Torres E. Troja Y. Uchiyama 30 Y. Yuan 31 S. Zimmer 32
Abstract : On 2015 June 16, Fermi-LAT observed a giant outburst from the flat spectrum radio quasar 3C 279 with a peak $>100$ MeV flux of $\sim3.6\times10^{-5}\;{\rm photons}\;{\rm cm}^{-2}\;{\rm s}^{-1}$ averaged over orbital period intervals. It is the historically highest $\gamma$-ray flux observed from the source including past EGRET observations, with the $\gamma$-ray isotropic luminosity reaching $\sim10^{49}\;{\rm erg}\;{\rm s}^{-1}$. During the outburst, the Fermi spacecraft, which has an orbital period of 95.4 min, was operated in a special pointing mode to optimize the exposure for 3C 279. For the first time, significant flux variability at sub-orbital timescales was found in blazar observations by Fermi-LAT. The source flux variability was resolved down to 2-min binned timescales, with flux doubling times less than 5 min. The observed minute-scale variability suggests a very compact emission region at hundreds of Schwarzschild radii from the central engine in conical jet models. A minimum bulk jet Lorentz factor ($\Gamma$) of 35 is necessary to avoid both internal $\gamma$-ray absorption and super-Eddington jet power. In the standard external-radiation-Comptonization scenario, $\Gamma$ should be at least 50 to avoid overproducing the synchrotron-self-Compton component. However, this predicts extremely low magnetization ($\sim5\times10^{-4}$). Equipartition requires $\Gamma$ as high as 120, unless the emitting region is a small fraction of the dissipation region. Alternatively, we consider $\gamma$ rays originating as synchrotron radiation of $\gamma_{\rm e}\sim1.6\times10^6$ electrons, in magnetic field $B\sim1.3$ kG, accelerated by strong electric fields $E\sim B$ in the process of magnetoluminescence. At such short distance scales, one cannot immediately exclude production of $\gamma$ rays in hadronic processes.
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Markus Ackermann, R. Anantua, K. Asano, Luca Baldini, Guido Barbiellini, et al.. Minute-Timescale >100 MeV gamma-ray variability during the giant outburst of quasar 3C 279 observed by Fermi-LAT in 2015 June. The Astrophysical journal letters, Bristol : IOP Publishing, 2016, 824 (L20), 8 p. ⟨10.3847/2041-8205/824/2/L20⟩. ⟨insu-01360099⟩



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