140 research outputs found
Magnetic Field Amplification and Blazar Flares
Recent multiwavelength observations of PKS 0208-512 by SMARTS, Fermi, and
Swift revealed that gamma-ray and optical light curves of this flat spectrum
radio quasars are highly correlated, but with an exception of one large optical
flare having no corresponding gamma-ray activity or even detection. On the
other hand, recent advances in SNRs observations and plasma simulations both
reveal that magnetic field downstream of astrophysical shocks can be largely
amplified beyond simple shock compression. These amplifications, along with
their associated particle acceleration, might contribute to blazar flares,
including the peculiar flare of PKS 0208-512. Using our time dependent
multizone blazar emission code, we evaluate several scenarios that may
represent such phenomena. This code combines Monte Carlo method that tracks the
radiative processes including inverse Compton scattering, and Fokker-Planck
equation that follows the cooling and acceleration of particles. It is a
comprehensive time dependent code that fully takes into account the light
travel time effects. In this study, both the changes of the magnetic field and
acceleration efficiency are explored as the cause of blazar flares. Under these
assumption, synchrotron self-Compton and external Compton scenarios produce
distinct features that favor the external Compton scenario. The optical flares
with/without gamma-ray counterparts can be explained by different allocations
of energy between the magnetization and particle acceleration, which in turn
can be affected by the relative orientation between the magnetic field and the
shock flow. We compare the details of the observations and simulation, and
highlight what implications this study has on our understanding of relativistic
jets.Comment: 6 pages. To appear in the proceeding of 'The Innermost Regions of
Relativistic Jets and Their Magnetic Fields', Granada, Spai
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Magnetic Field Amplification and Flat Spectrum Radio Quasars
We perform time-dependent, spatially-resolved simulations of blazar emission
to evaluate several flaring scenarios related to magnetic-field amplification
and enhanced particle acceleration. The code explicitly accounts for
light-travel-time effects and is applied to flares observed in the flat
spectrum radio quasar (FSRQ) PKS 0208-512, which show optical/{\gamma}-ray
correlation at some times, but orphan optical flares at other times. Changes in
both the magnetic field and the particle acceleration efficiency are explored
as causes of flares. Generally, external Compton emission appears to describe
the available data better than a synchrotron self-Compton scenario, and in
particular orphan optical flares are difficult to produce in the SSC framework.
X-ray soft-excesses, {\gamma}-ray spectral hardening, and the detections at
very high energies of certain FSRQs during flares find natural explanations in
the EC scenario with particle acceleration change. Likewise, optical flares
with/without {\gamma}-ray counterparts can be explained by different
allocations of energy between the magnetization and particle acceleration,
which may be related to the orientation of the magnetic field relative to the
jet flow. We also calculate the degree of linear polarization and polarization
angle as a function of time for a jet with helical magnetic field. Tightening
of the magnetic helix immediately downstream of the jet perturbations, where
flares occur, can be sufficient to explain the increases in the degree of
polarization and a rotation by >= 180 degree of the observed polarization
angle, if light-travel-time effects are properly considered.Comment: 12 pages, 9 figures. Accepted for publication in MNRA
SMARTS OPTICAL AND INFRARED MONITORING OF 12 GAMMA-RAY BRIGHT BLAZARS
We present multiwavelength data for 12 blazars observed from 2008 to 2010 as part of an ongoing optical–infrared
photometric monitoring project. Sources were selected to be bright, southern (δ < 20◦) blazars observed by the
Fermi Gamma-Ray Space Telescope. Light curves are presented for the 12 blazars in BVRJK at near-daily cadence.
We find that optical and infrared fluxes are well correlated in all sources. Gamma-ray bright flat spectrum radio
quasars (FSRQs) in our sample have optical/infrared emission correlated with gamma-rays consistent with inverse
Compton-scattering models. In FSRQs, variability amplitude increases toward IR wavelengths, consistent with the
presence of a thermal accretion disk varying on significantly longer timescales than the jet. In BL Lac objects,
variability is mainly constant, or increases toward shorter wavelength. FSRQs have redder optical–infrared colors
when they are brighter,whileBLLac objects showno such trend. Several objects showcomplicated color–magnitude
behavior: AO 0235+164 appears in two different states depending on its gamma-ray intensity. OJ 287 and 3C 279
show some hysteresis tracks in their color–magnitude diagrams. Individual flares may be achromatic or otherwise
depart from the trend, suggesting different jet components becoming important at different times. We present a
time-dependent spectral energy distribution of the bright FSRQ 3C 454.3 during its 2009 December flare, which is
well fit by an external Compton model in the bright state, although day-to-day changes pose challenges to a simple
one-zone model. All data from the SMARTS monitoring program are publicly available on our Web site
Outcomes of Abrupt Switch to Bevacizumab of Patients Undergoing Aflibercept Intravitreal Injections for Neovascular Age-Related Macular Degeneration in a Tertiary Center in Lombardy, Italy: A Real-Life Retrospective Analysis
To assess real-life anatomical and functional outcomes of switch to bevacizumab in patients undergoing aflibercept intravitreal injections for nAMD
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