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Published in 2021 at "Universe"
DOI: 10.3390/universe7120472
Abstract: PSR B1259-63 is a γ-ray binary system, where the compact object is a pulsar. The system has an orbital period of 1236.7 days and shows peculiar γ-ray flares (in 100 MeV–300 GeV) after its periastron…
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Keywords:
psr b1259;
periastron passage;
periastron;