Spin Period Evolution of Vela Pulsar Based on the Wind Emission: Application to the Long Period Radio Pulsars GPM J1839‐10 (P = 21 Min) and GLEAM‐X J1627 (P = 18 Min)
ASTRONOMISCHE NACHRICHTEN（2024）
Key words
pulsars: general,pulsars: individual,PSR B0833-45(the Vela pulsar),stars: neutron,supernovae: individual
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