Image Details
Caption: Figure 6.
The half-opening angle of the wider component θj,w (in degrees) as a function of the jet break tj,w (days) and isotropic-equivalent kinetic energy Ek,iso,w (erg). The dashed lines indicate the combinations of tj,w and Ek,iso,w that will yield θj,w of 45°, 60°, and 75°. We assume here the redshift and CBM density from Equation (9), effectively performing a relative scaling from the 2﹩\mathop{.}\limits^{\unicode{x000b0}}﹩1 narrow jet.
© 2026. The Author(s). Published by the American Astronomical Society.