Spinar model for the fast-rotating collapsing objects
February 25, 2021
After observing the kilonova in the optical range, one of the most interesting tasks of astronomy is to observe a short gamma-ray burst that can be formed when neutron stars merge. Using the spinar paradigm, we model this process to evaluate the possibility of such observations by a network of robotic optical telescopes MASTER. We show that, despite the obvious complexity of such observations, the MASTER may be able to make them.
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