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Spider pulsars are millisecond pulsars (MSPs) with low-mass companions in short-period orbits (Fruchter et al. 1988; Roberts 2013). They are descendants of low-mass X-ray binaries after accretion onto the pulsar has terminated (Archibald et al. 2009; Stappers et al. 2014). Redbacks (RBs) and black widows (BWs) are two types of spider pulsars with different companion masses.
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