Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white-dwarfs

@inproceedings{Wang2022FormationOM,
  title={Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white-dwarfs},
  author={Bo Wang and Dongdong Liu and Hai-liang Chen},
  year={2022}
}
Accretion-induced collapse (AIC) of massive white-dwarfs (WDs) has been proposed as an important way for the formation of neutron star (NS) systems. An oxygen-neon (ONe) WD that accretes H-rich material from a red-giant (RG) star may experience the AIC process, eventually producing millisecond pulsars (MSPs), known as the RG donor channel. Previous studies indicate that this channel can only account for MSPs with orbital periods > 500 d. It is worth noting that some more MSPs with wide orbits… 
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