Secondary pairs from Bethe-Heitler interactions of relativistic protons in ULX funnels can produce 0.1-100 MeV emission at 10^34 to 10^38 erg/s, a testable hadronic signature.
The content of astrophysical jets
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
abstract
Jets, collimated outflows of particles and fields, are observed in a wide variety of astrophysical systems, including Active Galactic Nuclei of various types, microquasars, gamma-ray bursts, and young stellar objects. Despite intensive efforts along several decades of observational and theoretical research, there are still many uncertainties and open questions related to how jets are produced and what is their composition. In this review I offer an outline of some current views on the content and basic properties of astrophysical jets.
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Effects of Bethe-Heitler pair production in ultraluminous X-ray sources
Secondary pairs from Bethe-Heitler interactions of relativistic protons in ULX funnels can produce 0.1-100 MeV emission at 10^34 to 10^38 erg/s, a testable hadronic signature.