Image Details
Caption: Fig. 12.
Schematic depiction of the six possible ways in which the Lorentz factor at injection of those particles that ultimately contribute to the radiation we observe (emitted at tobs) may relate to the Lorentz factors at the breaks in the injected spectrum. As in Fig. 11, the light gray regions are where p = 2, the dark gray regions are where p = 3, and the white regions are where p = pm.
© 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.