Astrophysics

吸积毫秒X射线脉冲星

Accreting Millisecond X-ray Pulsar

A rapidly rotating neutron star that has been spun up by accretion of matter from a companion star. It exhibits pulsed X-ray emission due to its strong magnetic field and rotation. / 一种由伴星物质吸积被加速旋转的中子星。由于其强磁场和自转，它表现出脉冲X射线发射。

Knowledge type: 自然理论
First proposed or discovered
Proposer: Turkey Farm member
Creator: 农场主
Last updated: 2026-10-31 17:07:03

Sub-knowledge points

Spin-up mechanismX-ray pulsationsType-II-like bursts

Higher-order knowledge points

Neutron starsX-ray binaries

Main parameters and performance indicators

Rotation Period: Typically millisecondsMass: ~1.4 Solar MassesMagnetic Field: Strong (10^8 - 10^12 Gauss)

Open problems

No unresolved problem recorded yet

Related literature

ranked by community stars

On the assessment of the disk truncation and detection of type-II-like bursts from the accreting millisecond X-ray pulsar IGR J17062–6143Open source

吸积毫秒X射线脉冲星

Sub-knowledge points

Higher-order knowledge points

Main parameters and performance indicators

Open problems

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