AN ANALYSIS OF CHANDRA DEEP FOLLOW-UP GAMMA-RAY BURSTS: IMPLICATIONS FOR OFF-AXIS JETS
Journal Article
·
· Astrophysical Journal
- Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States)
- Alexander von Humboldt Fellow, Max-Planck Institute for Extraterrestrial Physics (MPE), Postfach 1312, D-85741 Garching (Germany)
- Center for Cosmology and Particle Physics, Physics Department, New York University, New York, NY 10003 (United States)
- Department of Physics and Astronomy, University of Leicester, Leicester, LE1 7RH (United Kingdom)
- NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
We present a sample of 27 gamma-ray bursts (GRBs) with detailed Swift light curves supplemented by late-time Chandra observations. To answer the missing jet-break problem in general, we develop a numerical-simulation-based model that can be directly fit to the data using Monte Carlo methods. Our numerical model takes into account all the factors that can shape a jet break: (i) lateral expansion, (ii) edge effects, and (iii) off-axis effects. Our results provide improved fits to the light curves and constraints on physical parameters. More importantly, our results suggest that off-axis effects are important and must be included in interpretations of GRB jet breaks.
- OSTI ID:
- 22522346
- Journal Information:
- Astrophysical Journal, Vol. 806, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
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