Relativistic jets in active galactic nuclei and microquasars

GE Romero, M Boettcher, S Markoff… - Space Science Reviews, 2017 - Springer
Collimated outflows (jets) appear to be a ubiquitous phenomenon associated with the
accretion of material onto a compact object. Despite this ubiquity, many fundamental physics …

Progress in multi-wavelength and multi-messenger observations of blazars and theoretical challenges

M Böttcher - Galaxies, 2019 - mdpi.com
This review provides an overview of recent advances in multi-wavelength and multi-
messenger observations of blazars, the current status of theoretical models for blazar …

Relativistic reconnection: an efficient source of non-thermal particles

L Sironi, A Spitkovsky - The Astrophysical Journal Letters, 2014 - iopscience.iop.org
In magnetized astrophysical outflows, the dissipation of field energy into particle energy via
magnetic reconnection is often invoked to explain the observed non-thermal signatures. By …

Turbulent, extreme multi-zone model for simulating flux and polarization variability in blazars

AP Marscher - The Astrophysical Journal, 2013 - iopscience.iop.org
The author presents a model for variability of the flux and polarization of blazars in which
turbulent plasma flowing at a relativistic speed down a jet crosses a standing conical shock …

The internal-collision-induced magnetic reconnection and turbulence (ICMART) model of gamma-ray bursts

B Zhang, H Yan - The Astrophysical Journal, 2010 - iopscience.iop.org
The recent Fermi observation of GRB 080916C shows that the bright photosphere emission
associated with a putative fireball is missing, which suggests that the central engine likely …

Relativistic jets shine through shocks or magnetic reconnection?

L Sironi, M Petropoulou… - Monthly Notices of the …, 2015 - academic.oup.com
Observations of gamma-ray-bursts and jets from active galactic nuclei reveal that the jet flow
is characterized by a high radiative efficiency and that the dissipative mechanism must be a …

Particle acceleration and plasma dynamics during magnetic reconnection in the magnetically dominated regime

F Guo, YH Liu, W Daughton, H Li - The Astrophysical Journal, 2015 - iopscience.iop.org
Magnetic reconnection is thought to be the driver for many explosive phenomena in the
universe. The energy release and particle acceleration during reconnection have been …

A possible relativistic jetted outburst from a massive black hole fed by a tidally disrupted star

JS Bloom, D Giannios, BD Metzger, SB Cenko… - Science, 2011 - science.org
Gas accretion onto some massive black holes (MBHs) at the centers of galaxies actively
powers luminous emission, but most MBHs are considered dormant. Occasionally, a star …

[HTML][HTML] ASTRI Mini-Array core science at the Observatorio del Teide

S Vercellone, C Bigongiari, A Burtovoi… - Journal of High Energy …, 2022 - Elsevier
Abstract The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project led by
the Italian National Institute for Astrophysics (INAF) is developing and will deploy at the …

General physical properties of bright Fermi blazars

G Ghisellini, F Tavecchio, L Foschini… - Monthly Notices of …, 2010 - academic.oup.com
We studied all blazars of known redshift detected by the Fermi satellite during its first 3-
month survey. For the majority of them, pointed Swift observations ensure a good …