[HTML][HTML] Numerical simulations of jets

S Komissarov, O Porth - New Astronomy Reviews, 2021 - Elsevier
When astrophysical jets were discovered one hundred years ago, the field of numerical
simulations did not yet exit. Since the arrival of programmable computers though, numerical …

Relativistic jets of blazars

T Hovatta, E Lindfors - New Astronomy Reviews, 2019 - Elsevier
Relativistic jets of active galactic nuclei have been known to exist for 100 years. Blazars with
their jet pointing close to our line of sight are some of the most variable and extreme objects …

The nuclear spectroscopic telescope array (NuSTAR) high-energy X-ray mission

FA Harrison, WW Craig, FE Christensen… - The Astrophysical …, 2013 - iopscience.iop.org
ABSTRACT The Nuclear Spectroscopic Telescope Array (NuSTAR) mission, launched on
2012 June 13, is the first focusing high-energy X-ray telescope in orbit. NuSTAR operates in …

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 …

Extragalactic background light inferred from AEGIS galaxy-SED-type fractions

A Dominguez, JR Primack, DJ Rosario… - Monthly Notices of …, 2011 - academic.oup.com
The extragalactic background light (EBL) is of fundamental importance both for
understanding the entire process of galaxy evolution and for γ-ray astronomy, but the overall …

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 …

A hadronic origin for ultra-high-frequency-peaked BL Lac objects

M Cerruti, A Zech, C Boisson… - Monthly Notices of the …, 2015 - academic.oup.com
Current Cherenkov telescopes have identified a population of ultra-high-frequency peaked
BL Lac objects (UHBLs), also known as extreme blazars, that exhibit exceptionally hard TeV …

TXS 0506+ 056, the first cosmic neutrino source, is not a BL Lac

P Padovani, F Oikonomou… - Monthly Notices of …, 2019 - academic.oup.com
We present evidence that TXS 0506+ 056, the first plausible non-stellar neutrino source,
despite appearances, is not a blazar of the BL Lac type but is instead a masquerading BL …

Acceleration of particles at the termination shock of a relativistic striped wind

L Sironi, A Spitkovsky - The Astrophysical Journal, 2011 - iopscience.iop.org
The relativistic wind of obliquely rotating pulsars consists of toroidal stripes of opposite
magnetic field polarity, separated by current sheets of hot plasma. By means of two-and …

A change in the optical polarization associated with a γ-ray flare in the blazar 3C 279

Nature, 2010 - nature.com
It is widely accepted that strong and variable radiation detected over all accessible energy
bands in a number of active galaxies arises from a relativistic, Doppler-boosted jet pointing …