Titlebook: Neutron Stars and Their Birth Events; Wolfgang Kundt Book 1990 Kluwer Academic Publishers 1990 Accretion.Population.Supernova.accretion di

Irascible

Minikin

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

,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).

貿(mào)易

圖表證明

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

,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).