We investigate the number of gamma-ray bursts in two particular strips of the sky using the data in 3B catalog of Burst and Transient Source Experiment ( BATSE ) .
One stripe is related to the plane in which the intergalactic globular clusters ( R > 25kpc ) and Galactic satellite galaxies ( 45kpc < R < 280kpc ) concentrate , the other is concerned to nearby galaxies ( 1Mpc < R < 11Mpc ) .
We find that the density of GRBs in these two strips is higher than that in other parts of the sky with significance 2.8 and 1.9 \sigma respectively .
We also compare the peak flux distribution of GRBs in these two stripes with that in other parts of the sky , and find no difference in the former stripe but a difference in the latter with a significant level \alpha = 0.05 .
This is consistent with the distance scales of these two planes .
So it suggests that at least a substantial fraction of GRBs may be related to those objects in these two planes and thus originate within 11 Mpc .