Searching Ultra-compact Pulsar Binaries with Abnormal Timing Behavior

Ultra-compact pulsar binaries are both ideal sources of gravitational radiation for gravitational wave detectors and laboratories for fundamental physics. However, the shortest orbital period of all radio pulsar binaries is currently 1.6 hr. The absence of pulsar binaries with a shorter orbital peri...

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Veröffentlicht in:	The Astrophysical journal 2018-03, Vol.855 (1), p.35
Hauptverfasser:	Gong, B. P., Li, Y. P., Yuan, J. P., Tian, J., Zhang, Y. Y., Li, D., Jiang, B., Li, X. D., Wang, H. G., Zou, Y. C., Shao, L. J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Astrophysics binaries: general Binary stars Companion stars Computer simulation Dwarf stars Gravitational waves Gravity waves Noise prediction Optical counterparts (astronomy) Orbital elements Orbits Pulsars pulsars: individual (PSR B0919+06) Radiation Searching Tidal effects White dwarf stars
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