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1
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79960102295
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-
note
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-1/2 ≈ 10, with velocity v = βc of the jetted outflow (c is the speed of light in vacuum).
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-
-
-
5
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-
1542390387
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G. Fossati, L. Maraschi, A. Celotti, A. Comastri, G. Ghisellini, Mon. Not. R. Astron. Soc. 299, 433 (1998).
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(1998)
Mon. Not. R. Astron. Soc.
, vol.299
, pp. 433
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-
Fossati, G.1
Maraschi, L.2
Celotti, A.3
Comastri, A.4
Ghisellini, G.5
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6
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0039686312
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M. J. Rees, Nature 333, 523 (1988).
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(1988)
Nature
, vol.333
, pp. 523
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-
Rees, M.J.1
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11
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79960076987
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note
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-1.
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-
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19
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79960103760
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GCN Circular 11823, NASA Goddard Space Flight Center, Greenbelt, MD
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J. R. Cummings et al., "GRB 110328A: Swift detection of a burst" (GCN Circular 11823, NASA Goddard Space Flight Center, Greenbelt, MD, 2011).
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(2011)
GRB 110328A: Swift Detection of A Burst
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Cummings, J.R.1
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20
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79960080590
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A. J. Levan et al., Science 333, 199 (2011).
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(2011)
Science
, vol.333
, pp. 199
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Levan, A.J.1
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21
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79960103934
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GCN Circular 11847, NASA Goddard Space Flight Center, Greenbelt, MD
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J. S. Bloom, N. R. Butler, S. B. Cenko, D. A. Perley, "GRB 110328A / Swift J164449.3+573451: X-ray analysis and a mini-blazar analogy" (GCN Circular 11847, NASA Goddard Space Flight Center, Greenbelt, MD, 2011).
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(2011)
GRB 110328A / Swift J164449.3+573451: X-ray Analysis and A Mini-blazar Analogy
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Bloom, J.S.1
Butler, N.R.2
Cenko, S.B.3
Perley, D.A.4
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22
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79960098055
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-
note
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Interpretations similar to that in (21) were put forward later (23).
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-
-
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25
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79960088775
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note
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Within the uncertainties from Hubble imaging [∼300 pc; (20)], the central stellar and gas density could be high enough to allow other progenitors, such as supernovae.
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-
-
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28
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79960093717
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note
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As in gamma-ray burst light curves, even in the presence of relativistic motion, the observed variability should track that of the energy injection time scales from the central engine. Shorter time scale variability could, however, result from compact emitting regions moving fast within the jet (29).
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-
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33
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0000884638
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M. Spada, G. Ghisellini, D. Lazzati, A. Celotti, Mon. Not. R. Astron. Soc. 325, 1559 (2001).
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(2001)
Mon. Not. R. Astron. Soc.
, vol.325
, pp. 1559
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Spada, M.1
Ghisellini, G.2
Lazzati, D.3
Celotti, A.4
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34
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79960093260
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note
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This situation is not encountered in normal (long-lived) blazars because a large ≳kiloparsec-scale cavity has been carved by the preceding outflow.
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-
-
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35
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79960097705
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note
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Here the departure from the blazar analogy is worth noting, in that the physics of the radio emission is likely to be different in this case: We have suggested that the emission is originating from the shocked surrounding material (forward shock), not the shocked jet as in normal blazars, which could contain large-scale fields. Even so, only 10% of flat-spectrum radio quasars and BL Lac objects have polarization larger than our VLBI limits (36).
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-
-
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41
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79960084749
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note
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⊙ MBH). As in the orange model, the x-ray emission is dominated by external Compton scattering, whereas the peak at high energies results from synchrotron self-Compton emission. An additional synchrotron component from a mildly relativistic blast-wave afterglow at larger radius is invoked to explain the bright radio and millimeter fluxes.
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-
-
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42
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79960075935
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GCN Circular 11851, NASA Goddard Space Flight Center, Greenbelt, MD
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S. Campana, L. Foschini, G. Tagliaferri, G. Ghisellini, S. Covino, "GRB 110328/Swift J164449.3+573451: Fermi observations" (GCN Circular 11851, NASA Goddard Space Flight Center, Greenbelt, MD, 2011).
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(2011)
GRB 110328/Swift J164449.3+573451: Fermi Observations
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Campana, S.1
Foschini, L.2
Tagliaferri, G.3
Ghisellini, G.4
Covino, S.5
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43
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79960105980
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note
-
Although we have modeled the "quiescent" SED, a similar external Compton model can be made to fit the "flaring" x-ray state, provided that the jet luminosity is accordingly increased.
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-
-
-
45
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79960104130
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note
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⊙.
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|