We review the various ways in which binary pulsars, millisecond pulsars and pulsars in
globular clusters may have formed. To this end the formation processes of neutron stars in …

There is a wide range of fundamental physical problems directly related to how pulsars
function. Some of these are independent of the specific pulsar mechanism. Others relate …

A whole decades research collated, organised and synthesised into one single book!
Following a 60-page review of the seminal treatises of Misner, Thorne, Wheeler and …

The model comprises a rotating neutron star (R 106 cm) with a strong magnetic field (B 1012
gauss). Magnetic-field lines which reach the light cylinder are open field lines which connect …

THE spatial and luminosity distribution of γ-ray bursts as observed by the BATSE instrument
on the Compton Gamma Ray Observatory1, 2 provides support for the revival of the idea3, 4 …

The constancy of frequency in the recently discovered pulsed radio sources can be
accounted for by the rotation of a neutron star. Because of the strong magnetic fields and …

Kenneth Lang's classic work Astrophysical Formulae.(Vol. I and II) is now available as soft
cover edition in a set. This volume is a reference source of fundamental formulae in physics …

This book represents the first comprehensive treatment of the subject, covering the
theoretical principles, present experimental status and important applications of short-pulse …

Disk-Accretion onto a Black Hole. Time-Averaged Structure of Accretion Disk ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …

The radio properties of 4C21. 53 have been an enigma for many years. First, the object
displays interplanetary scintillations (IPS) at 81 MHz, indicating structure smaller than 1 are …