Abstract Deep optical images of small γ-ray burst error regions have generally resulted in the detection of several faint (mv ⋟ 22) sources in each error region. It may be possible to identify the neutron star source of a GRB on the basis of a high transverse peculiar velocity if the source is at moderate distance (∼ 100 pc). We report the results of searches for high proper motion objects in the error regions of GBS1412+78 (13 June 1979 /1,14/) and GBS2251-02 (5 November 1979 /2/).
A search for high proper motion objects in two γ-ray burst error regions
Advances in Space Research ; 6 , 4 ; 75-78
1986-01-01
4 pages
Article (Journal)
Electronic Resource
English
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