Simulations demonstrate that mega-parsec giant radio sources form successfully in normal hot baryonic gas environments within 10^13 to 10^15 solar mass dark matter halos, with radio powers matching observations.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2representative citing papers
Triaxial orbit modelling of integrated kinematic maps recovers the Sgr A* mass and shows the nuclear structures are mildly triaxial with radially varying orbit types.
citing papers explorer
-
Formation of mega-parsec giant radio sources from hosts residing in dark matter halos with normal hot baryonic gas fractions
Simulations demonstrate that mega-parsec giant radio sources form successfully in normal hot baryonic gas environments within 10^13 to 10^15 solar mass dark matter halos, with radio powers matching observations.