The 2015 outburst of the accreting millisecond pulsar IGR J17511–3057 as seen by INTEGRAL,Swift, andXMM-Newton

Author:

Papitto A.,Bozzo E.,Sanchez-Fernandez C.,Romano P.,Torres, D. F.,Ferrigno C.,Kajava J. J. E.,Kuulkers E.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 7 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. On the lack of X-ray pulsation in most neutron star low-mass X-ray binaries;Monthly Notices of the Royal Astronomical Society;2024-06-27

2. Constraints on the magnetic field structure in accreting compact objects from aperiodic variability;Monthly Notices of the Royal Astronomical Society;2022-07-01

3. Accretion Powered X-ray Millisecond Pulsars;Astrophysics and Space Science Library;2021-11-26

4. Indications of non-conservative mass transfer in AMXPs;Astronomy & Astrophysics;2019-07

5. NuSTARandXMM–Newtonbroad-band spectrum of SAX J1808.4–3658 during its latest outburst in 2015;Monthly Notices of the Royal Astronomical Society;2018-11-03

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