תקציר
Early X-ray afterglows recently detected by Swift frequently show a phase of very shallow flux decay lasting from ∼102.5 up to ∼10 4 s, followed by a steeper, more familiar decay. We suggest that the flat early part of the light curve may be a combination of (1) the decaying tail of the prompt emission and (2) the delayed onset of the afterglow emission observed from viewing angles slightly outside the edge of that part of the jet that generates prominent afterglow emission, as predicted previously. This would imply that a significant fraction of viewers get very little external shock energy along their line of sight and, therefore, see a very high γ-ray-to-kinetic energy ratio at early times. The early flat phase in the afterglow light curve implies, for standard afterglow theory, a very large γ-ray efficiency, typically ≳90%, which is very difficult to extract from baryons by internal shocks.
| שפה מקורית | אנגלית |
|---|---|
| עמודים (מ-עד) | L5-L8 |
| כתב עת | Astrophysical Journal |
| כרך | 641 |
| מספר גיליון | 1 II |
| מזהי עצם דיגיטלי (DOIs) | |
| סטטוס פרסום | פורסם - 10 אפר׳ 2006 |
| פורסם באופן חיצוני | כן |
הערה ביבליוגרפית
Funding Information:The authors gratefully acknowledge a Center of Excellence grant from the Israel Science Foundation, a grant from the Israel-US Binational Science Foundation, and support from the Arnow Chair of Theoretical Astrophysics. This research was supported by the US Department of Energy under contract DE-AC03-76SF00515 (J. G.).