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SXP 1062 is an exceptional case of a young neutron star in a wind-fedhigh-mass X-ray binary associated with a supernova remnant. A uniquecombination of measured spin period, its derivative, luminosity and young agemakes this source a key probe for the physics of accretion and neutron starevolution. Theoretical models proposed to explain the properties of SXP 1062shall be tested with new data.

The slow X-ray pulsar SXP 1062 and associated supernova remnant in the Wing of the Small Magellanic Cloud