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Variability of active galactic nuclei
MH Ulrich, L Maraschi, CM Urry - Annual Review of Astronomy …, 1997 - annualreviews.org
▪ Abstract A large collective effort to study the variability of active galactic nuclei (AGN) over
the past decade has led to a number of fundamental results on radio-quiet AGN and blazars …
the past decade has led to a number of fundamental results on radio-quiet AGN and blazars …
Relativistic jets in active galactic nuclei and microquasars
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 …
accretion of material onto a compact object. Despite this ubiquity, many fundamental physics …
A unifying view of the spectral energy distributions of blazars
G Fossati, L Maraschi, A Celotti… - Monthly Notices of …, 1998 - academic.oup.com
We collect data at well-sampled frequencies from the radio to the γ-ray range for the
following three complete samples of blazars: the Slew survey, the 1-Jy samples of BL Lacs …
following three complete samples of blazars: the Slew survey, the 1-Jy samples of BL Lacs …
A possible relativistic jetted outburst from a massive black hole fed by a tidally disrupted star
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 …
powers luminous emission, but most MBHs are considered dormant. Occasionally, a star …
A theoretical unifying scheme for gamma‐ray bright blazars
G Ghisellini, A Celotti, G Fossati… - Monthly Notices of …, 1998 - Wiley Online Library
The phenomenology of γ‐ray bright blazars can be accounted for by a sequence in the
source power and intensity of the diffuse radiation field surrounding the relativistic jet …
source power and intensity of the diffuse radiation field surrounding the relativistic jet …
Non-thermal particle acceleration in collisionless relativistic electron–proton reconnection
GR Werner, DA Uzdensky… - Monthly Notices of …, 2018 - academic.oup.com
Magnetic reconnection in relativistic collisionless plasmas can accelerate particles and
power high-energy emission in various astrophysical systems. Whereas most previous …
power high-energy emission in various astrophysical systems. Whereas most previous …
Canonical high-power blazars
G Ghisellini, F Tavecchio - Monthly Notices of the Royal …, 2009 - academic.oup.com
The jets of powerful blazars propagate within relatively dense regions of radiation produced
externally to the jet. This radiation is a key ingredient to understand the origin of the high …
externally to the jet. This radiation is a key ingredient to understand the origin of the high …
A multimessenger study of the blazar PKS 0735+ 178: a new major neutrino source candidate
The blazar PKS 0735+ 178 is possibly associated with multiple neutrino events observed by
the IceCube, Baikal, Baksan, and KM3NeT neutrino telescopes while it was flaring in the γ …
the IceCube, Baikal, Baksan, and KM3NeT neutrino telescopes while it was flaring in the γ …
Variable very high energy γ-ray emission from Markarian 501
The blazar Mrk 501 was observed at energies above 0.10 TeV with the MAGIC Telescope
from 2005 May through July. The high sensitivity of the instrument enabled the determination …
from 2005 May through July. The high sensitivity of the instrument enabled the determination …
The power of relativistic jets is larger than the luminosity of their accretion disks
G Ghisellini, F Tavecchio, L Maraschi, A Celotti… - Nature, 2014 - nature.com
Theoretical models for the production of relativistic jets from active galactic nuclei predict that
jet power arises from the spin and mass of the central supermassive black hole, as well as …
jet power arises from the spin and mass of the central supermassive black hole, as well as …