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| Query : 2009ApJ...691L..37R |
2009ApJ...691L..37R - Astrophys. J., 691, L37-L40 (2009/January-3)
Prompt TeV emission from cosmic rays accelerated by gamma-ray bursts interacting with a surrounding stellar wind.
RAZZAQUE S., MENA O. and DERMER C.D.
Abstract (from CDS):
Protons accelerated in the internal shocks of a long-duration gamma-ray burst (GRB) can escape the fireball as cosmic rays by converting to neutrons. Hadronic interactions of these neutrons inside a stellar wind bubble created by the progenitor star will produce TeV γ-rays via neutral meson decay and synchrotron radiation by charged pion-decay electrons in the wind magnetic field. Such γ-rays should be observable from nearby GRBs by currently running and upcoming ground-based detectors.
Abstract Copyright: ∼
Journal keyword(s): gamma rays: bursts - gamma rays: theory - radiation mechanisms: non-thermal
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | GRB 941110 | gB | 16 06 | +47.7 | ~ | 24 | 0 | |||||
| 2 | GRB 970417A | gB | 19 21 | +54.2 | ~ | 56 | 0 |
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