Colliding compact objects

Details Colliding compact objects Colliding compact objects

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1133..115t&link_type=abstract

GAMMA-RAY BURST: Sixth Huntsville Symposium. AIP Conference Proceedings, Volume 1133, pp. 115-117 (2009).

Other

Gamma-Ray Sources, Gamma-Ray Bursts, Supernovae, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays

Scientific paper

We study the collisions of compact objects induced by neutron star (NS) birth kicks. If a binary system survives the first supernova (SN) explosion, in some cases the second SN may place the stellar remnants into bound highly eccentric orbits. The two compact objects will tidally interact and quickly spiral into each other. We expect such encounters to happen within a few days since the SN explosion, though a significant delay is also foreseen.

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