2012ApJ...749..100D

Query : 2012ApJ...749..100D

2012ApJ...749..100D - Astrophys. J., 749, 100 (2012/April-3)

Kinematic origin of correlations between gamma-ray burst observables.

DADO S. and DAR A.

Abstract (from CDS):

Recently, several new correlations between gamma-ray burst (GRB) observables have been discovered. Like previously well-established correlations, they challenge GRB models. Here, we show that in the cannonball (CB) model of GRBs, the newly discovered correlations have the same simple kinematic origin as those discovered earlier. They all result from the strong dependence of the observed radiations on the Lorentz and Doppler factors of the jet of highly relativistic plasmoids (CBs) that produces the observed radiations by interaction with the medium through which it propagates.

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Journal keyword(s): gamma-ray burst: general - gamma-ray burst: individual: 090529A

Simbad objects: 10

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Number of rows : 10
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 071031 gB 00 25 37.40 -58 03 33.9           ~ 184 0
2 GRB 080710 gB 00 33 05.68 +19 30 05.8           ~ 136 0
3 GRB 070318 gB 03 13 56.830 -42 56 46.30 18.27 16.23 15.49     ~ 170 0
4 GRB 060904B gB 03 52 50.520 -00 43 30.61 18.27 19.14 18.37     ~ 208 0
5 GRB 970508 gB 06 53 49.2 +79 16 19           ~ 883 1
6 GRB 080330 gB 11 17 06.70 +30 36 24.1           ~ 145 0
7 GRB 070419A gB 12 10 58.830 +39 55 34.06 18.52         ~ 130 0
8 GRB 070208 gB 13 11 32.607 +61 57 54.37 20.79 20.79 19.86     ~ 119 0
9 GRB 090529A gB 14 09 52.56 +24 27 32.2           ~ 23 0
10 GRB 071010A gB 19 12 14.42 -32 24 06.2           ~ 138 0

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