Accretion by rotating magnetic neutron stars. I - Flow of matter inside the magnetosphere and its implications for spin-up and spin-down of the star-Reference-Cited by-同舟云学术

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Accretion by rotating magnetic neutron stars. I - Flow of matter inside the magnetosphere and its implications for spin-up and spin-down of the star

Published:1977-10 Issue: Volume:217 Page:578
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Ghosh P.,Pethick C. J.,Lamb F. K.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 190 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Measuring the Magnetic Dipole Moment and Magnetospheric Fluctuations of Accretion-powered Pulsars in the Small Magellanic Cloud with an Unscented Kalman Filter;The Astrophysical Journal;2024-08-01

2. Measuring the Magnetic Dipole Moment and Magnetospheric Fluctuations of SXP 18.3 with a Kalman Filter;The Astrophysical Journal;2024-04-01

3. Gravitational waves from neutron-star mountains;Classical and Quantum Gravity;2024-01-23

4. A global 3D simulation of magnetospheric accretion – I. Magnetically disrupted discs and surface accretion;Monthly Notices of the Royal Astronomical Society;2023-12-04

5. Stable accretion in young stars: the cases of EX Lupi and TW Hya;Monthly Notices of the Royal Astronomical Society;2023-10-05

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