Image Details

Choose export citation format:

High-energy Emission Components in the Short GRB 090510

  • Authors: Alessandra Corsi, Dafne Guetta, and Luigi Piro

CORSI, GUETTA, & PIRO 2010 The Astrophysical Journal 720 1008.

  • Provider: AAS Journals

Caption: Figure 3.

Temporal evolution (black lines) of the Lorentz factor for the narrow (left panel) and wide (right panel) jet components. The red-dotted lines are plotted for comparison and correspond to the standard evolution Γ ∝ t −3/8 for an adiabatic fireball expanding in a uniform medium (e.g., Sari et al. 1998). The initial values Γ 0 are set to be 10 4 and 220 for the narrow and wide jet components, respectively. After t j , which is set to be ~1000 s for the narrow jet (corresponding to θ j ~ 0 fdg1) and ~2 × 10 4 s for the wide jet (corresponding to θ j ~ 0 fdg4), the Lorentz factor is evolved following a temporal scaling of Γ ∝ t −1/2 (e.g., Peng et al. 2005).

Other Images in This Article
Copyright and Terms & Conditions