Pair production via radiative magnetic reconnection near spinning black holes supplies non-uniform plasma to jets at levels sufficient to explain M87 radio emission.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2roles
background 1polarities
background 1representative citing papers
Stacked blazar data show strongest gamma-ray to radio correlation at a 180-day delay, with some sources displaying 1-3 year lags between activity in the two bands.
citing papers explorer
-
Non-uniform particle injection into black hole jets by radiative magnetic reconnection
Pair production via radiative magnetic reconnection near spinning black holes supplies non-uniform plasma to jets at levels sufficient to explain M87 radio emission.
-
Characterizing Gamma-Radio Delayed Flaring Activity from Blazars
Stacked blazar data show strongest gamma-ray to radio correlation at a 180-day delay, with some sources displaying 1-3 year lags between activity in the two bands.