Millisecond X-Ray Variability from an Accreting Neutron Star System-Reference-Cited by-同舟云学术

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Millisecond X-Ray Variability from an Accreting Neutron Star System

Published:1996-09-20 Issue:1 Volume:469 Page:L9-L12
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Strohmayer Tod E.,Zhang William,Swank Jean H.,Smale Alan,Titarchuk Lev,Day Charles,Lee Umin

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference28 articles.

1. Is GX5 – 1 a millisecond pulsar?

2. Photon bubbles - Overstability in a magnetized atmosphere

3. X-ray observations of the burst source MXB 1728 - 34

4. Propagation of nuclear burning fronts on accreting neutron stars: X-ray bursts and sub-hertz noise

5. Spectral Properties of Accretion Disks around Galactic and Extragalactic Black Holes

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1. Characterisation of the X-ray point source variability in the eROSITA south ecliptic pole field;Astronomy & Astrophysics;2024-06-28

2. Detection of Simultaneous Quasiperiodic Oscillation Triplets in 4U 1728-34 and Constraining the Neutron Star Mass and Moment of Inertia;The Astrophysical Journal;2024-05-28

3. Energy dependence of quasi-periodic oscillations in accreting X-ray pulsars;Monthly Notices of the Royal Astronomical Society;2024-05-02

4. Spin Evolution of Neutron Stars;Galaxies;2024-02-10

5. Low-Magnetic-Field Neutron Stars in X-ray Binaries;Handbook of X-ray and Gamma-ray Astrophysics;2024

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