Merger of Neutron Stars

Merger of Neutron Stars
(Credit: P.J.T. Leonard (NASA/GSFC))

Larger GIF version

One model for GRBs is a binary pair of neutron stars, with their orbital separation ground down by billions of years of gravitational radiation, finally merging to form a black hole. In the process of merging the neutron stars tear each other apart, forming an accretion disk and jets.



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Last modified: Thursday, 26-Jun-2003 13:48:47 EDT

HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.