Irascible
发表于 2025-4-1 04:05:12
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Minikin
发表于 2025-4-1 06:02:47
Five Lectures on Accretion-Driven Stellar X-Ray Sources, was a brief review on X-ray bursts, lecture #3 (by WHGL) was on the mass-radius relations of neutron stars, lecture #4 (by WHGL) was on the Rapid Burster, and lecture #5 (by JvP) was a brief review of quasi-periodic oscillations (QPO) in the X-ray flux of X-ray binaries.
Irremediable
发表于 2025-4-1 11:20:44
,Lecture #4 — the Rapid Burster (MXB 1730-335),nds to ∼ 1 hour). They behave like a relaxation oscillator: the time interval to the next burst is roughly proportional to the integrated flux in the previous burst (Lewin .. 1976). Attempts have been made to describe this recurrence behaviour of the Rapid Burster in terms of deterministic chaos (Celnikier 1977).
贸易
发表于 2025-4-1 18:00:26
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图表证明
发表于 2025-4-1 19:53:00
Neutron-Star Accretion,e, at its inner edge, should depend not only on the accretion rate and illumination but also on the spin inclination and obliquity of the magnetic dipole moment. An oscillating tilt angle may cause the superorbital period.
Abjure
发表于 2025-4-2 01:28:50
,Lecture #2 — X-Ray Bursts (Of Type 1),son of burst recurrence behaviour, as a function of the persistent X-ray luminosity, with expectations based on the thermonuclear flash model. For a comprehensive review of X-ray bursts, covering the entire field up to 1983, the reader is referred to Lewin & Joss (1981, 1983).