2006PASJ...58L...7A


Query : 2006PASJ...58L...7A

2006PASJ...58L...7A - Publ. Astron. Soc. Jap., 58, L7-L10 (2006/February-0)

Possibility of ultra high-energy cosmic rays from the giant flare in soft gamma repeater 1806-20.

ASANO K., YAMAZAKI R. and SUGIYAMA N.

Abstract (from CDS):

begin{HTML} On 2004 December 27, a giant flare from the soft gamma repeater 1806-20 was observed. The radiation mechanism of the initial peak of the flare would be controversial. In this letter we point out that very high-energy cosmic rays would be produced in the case that the flare was caused by internal shocks, as is usually considered for gamma-ray bursts. The highest energy of cosmic rays can reach 10<sup>19</sup><sub>eV</sub>, if the Lorentz factor of the shocks is sufficiently high. Future observations of cosmic rays will inform us about the mechanism of the giant flare.

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Journal keyword(s): cosmic rays - gamma-rays: bursts - pulsars: individual: SGR 1806-20

Simbad objects: 4

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Number of rows : 4
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 PSR B0525-66 Psr 05 26 00.7 -66 04 35           ~ 569 1
2 V* RZ Com SB* 12 35 05.0595351864 +23 20 14.027775864   11.09 10.57 10.082 9.77 G0Vn 202 0
3 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1316 2
4 NAME Sgr 1900-14 Rad 19 03 33.058 -13 57 54.76           ~ 16 1

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