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List of illustrations | p. xi |
Preface | p. xxvii |
The discovery of pulsars | p. 1 |
The radio discovery | p. 2 |
Interplanetary scintillation | p. 3 |
The Nature letter of February 1968 | p. 5 |
Oscillations and orbits | p. 6 |
The identification with neutron stars | p. 9 |
Optical pulses from the Crab Pulsar | p. 10 |
X-ray pulses from the Crab Pulsar | p. 11 |
Rotation periods | p. 11 |
The interstellar medium | p. 13 |
The population of pulsars | p. 14 |
Physics of the neutron star | p. 15 |
Neutron stars | p. 16 |
White dwarf stars | p. 17 |
Neutron stars | p. 17 |
Neutron star diameters | p. 20 |
Thermal radiation, luminosity and redshift | p. 20 |
The crust and the neutron fluid | p. 22 |
The magnetic fields of neutron stars | p. 23 |
The magnetosphere | p. 24 |
Telescopes and techniques | p. 27 |
Radio telescopes | p. 27 |
Infrared, optical and ultraviolet telescopes | p. 28 |
X-ray observations | p. 28 |
Gamma-ray space-based telescopes | p. 29 |
Imaging atmospheric Cerenkov telescopes | p. 32 |
Searching for periodic pulses | p. 33 |
Frequency dispersion in pulse arrival time | p. 35 |
De-dispersion | p. 37 |
The detection of binary pulsar systems | p. 39 |
Searches for millisecond pulsars | p. 41 |
Searches of supernova remnants and globular clusters | p. 42 |
The surveys for normal pulsars | p. 43 |
Sensitivity: selection effects | p. 45 |
Combatting radio interference | p. 47 |
Current and future surveys | p. 48 |
The distances of the pulsars | p. 49 |
Pulsar distances from parallax | p. 50 |
Kinematic distances | p. 52 |
Pulsar distances from neutral hydrogen absorption | p. 53 |
Pulsar distances from optical identifications | p. 54 |
Radio interstellar scattering | p. 57 |
The H II regions | p. 57 |
The model electron distribution | p. 58 |
The accuracy of the electron density model | p. 58 |
Pulsar timing | p. 61 |
Pulsar positions and the Earth's orbit | p. 62 |
The Römer correction to the barycentre | p. 64 |
The general relativistic corrections | p. 65 |
Fundamental positional reference frames | p. 66 |
Periods and period changes | p. 67 |
Proper motion | p. 68 |
Gravitational acceleration | p. 69 |
Precession | p. 70 |
Pulsar ages and the braking index | p. 71 |
Pulsars as standard clocks | p. 73 |
Timing and astrometry of binary pulsars | p. 76 |
Parameters of a binary orbit | p. 76 |
Annual orbital parallax | p. 79 |
Relativistic effects in binary orbits | p. 79 |
The relativistic evolution of a binary orbit | p. 80 |
The Double Pulsar binary J0737-3039A/B | p. 84 |
Tests of gravitational theory | p. 84 |
Gravitational waves | p. 85 |
The detection of planetary pulsar systems | p. 86 |
Timing irregularities | p. 88 |
Glitches | p. 89 |
The occurrence of glitches | p. 90 |
Slowdown rate after a glitch | p. 92 |
The exponential recoveries | p. 93 |
Changes of moment of inertia | p. 95 |
Two-component models: crust and superfluid | p. 96 |
Vorticity in the neutron fluid | p. 97 |
Pinning and unpinning | p. 98 |
Summary of glitch theory | p. 99 |
Alternative glitch theories | p. 99 |
Timing noise | p. 100 |
The origin of timing noise | p. 102 |
The Galactic population of pulsars | p. 105 |
The surveys | p. 105 |
The observed distribution of normal pulsars | p. 106 |
The derived luminosity and spatial distributions | p. 107 |
Pulsar velocities and ages | p. 110 |
The Galactic Centre region | p. 112 |
Model populations | p. 113 |
The pulsar birthrate | p. 114 |
The population of millisecond pulsars | p. 115 |
The Crab and Vela Pulsars | p. 117 |
Young pulsars | p. 117 |
Energy output | p. 117 |
The Crab Pulsar, PSRB0531+21 | p. 118 |
The Vela Pulsar, PSRB0833-45 | p. 128 |
Other young pulsars | p. 134 |
Characteristic ages | p. 134 |
Age from proper motion | p. 135 |
Uncertain ages: 3C58 and PSR J0205+6449 | p. 135 |
A Crab Pulsar look-alike: PSR B0540-69 | p. 136 |
An old SNR with a young pulsar: PSR B1509-58 | p. 136 |
A young, slow pulsar: PSR J1846-0258 in Kes 75 | p. 137 |
Gamma-rays but no radio: J0633+1746 (Geminga) | p. 137 |
The youngest pulsars | p. 138 |
Gamma-ray spectra | p. 139 |
Emitted power | p. 142 |
Braking indices | p. 144 |
Pulsar wind nebulae | p. 145 |
Millisecond and binary pulsars | p. 151f |
A distinct population | p. 151 |
Binary stars | p. 151 |
The discoveries | p. 153 |
The binaries and their orbits | p. 155 |
The masses of the binary pulsars and their companions | p. 156 |
Orbits and spin-up histories | p. 160 |
Pulsars with massive main-sequence companions | p. 163 |
The eclipsing millisecond binaries | p. 164 |
The globular cluster pulsars | p. 166 |
The magnetic fields of the millisecond pulsars | p. 168 |
The velocities of millisecond pulsars | p. 169 |
Accretion-powered X-ray pulsars | p. 170 |
Millisecond X-ray and radio pulsars | p. 172 |
Binary X-ray light curves | p. 172 |
Orbits and companion masses | p. 173 |
The high-mass X-ray binaries (HMXBs) | p. 174 |
The low-mass X-ray binaries (LMXBs) | p. 176 |
Peculiar systems, black holes and transients | p. 178 |
Spin-up, accretion and inertia | p. 178 |
Magnetic field strength | p. 179 |
The X-ray bursters | p. 180 |
The Rapid Burster | p. 182 |
Quasi-periodic (QPO) and kilohertz oscillations | p. 183 |
Magnetars | p. 184 |
The Soft Gamma-ray Repeaters (SGRs) | p. 184 |
The Anomalous X-ray Pulsars (AXPs) | p. 186 |
AXPs, SGRs, RRATs and XDINSs as magnetars | p. 187 |
Demography and origin of the magnetars | p. 189 |
Growth of the dipole field | p. 191 |
Supernovae and their remnants | p. 192 |
The nature of supernovae | p. 192 |
Stellar evolution and stellar collapse | p. 194 |
Accretion-induced supernova collapse | p. 195 |
Luminosity decay | p. 196 |
Frequency of occurrence of supernovae | p. 196 |
Supernova remnants | p. 198 |
The Crab Nebula | p. 200 |
The continuum radiation from the Crab Nebula | p. 202 |
The energy supply | p. 203 |
Pulsar wind nebulae | p. 205 |
Associations between pulsars and supernovae | p. 205 |
Integrated pulse profiles | p. 207 |
Integrated pulse widths | p. 207 |
The beam geometry | p. 209 |
Observed profile widths | p. 211 |
Radio frequency dependence | p. 211 |
Beam components, core and cone | p. 213 |
The overall beam shape | p. 216 |
The millisecond pulsars | p. 216 |
Notches | p. 217 |
Profile changing and mode changing | p. 218 |
Polarisation geometry | p. 219 |
Integrated polarisation profiles | p. 222 |
Orthogonal polarisation modes | p. 225 |
Position angle swing rates | p. 226 |
Millisecond pulsars | p. 226 |
Individual pulses | p. 230 |
Single pulse intensities and pulse nulling | p. 231 |
Rotating Radio Transient sources (RRATs) | p. 234 |
Sub-pulses | p. 234 |
Drifting and modulation | p. 234 |
Drift rates | p. 238 |
Drifting after nulling | p. 240 |
The polarisation of sub-pulses | p. 240 |
Microstructure and giant pulses | p. 243 |
Location of emitting regions | p. 245 |
Outer gap emission | p. 245 |
Sources of radio emission | p. 246 |
Polar cap emission | p. 247 |
Core and cone components | p. 251 |
Millisecond pulsars (MSPs) | p. 252 |
Primary emission beamwidth | p. 252 |
Aberration, retardation and magnetic field sweep-back | p. 253 |
Radio from the outer magnetosphere gap | p. 254 |
Radiation processes | p. 258 |
Cyclotron radiation | p. 258 |
Synchrotron radiation | p. 260 |
Curvature radiation | p. 262 |
The effect of a particle energy spectrum | p. 263 |
Self-absorption | p. 264 |
Inverse Compton radiation | p. 264 |
Maser amplification | p. 264 |
Coherence in the radio emission | p. 265 |
Relativistic beaming | p. 265 |
The emission mechanisms | p. 267 |
The two locations | p. 267 |
The outer gap: curvature and synchrotron radiation | p. 269 |
Radio spectra | p. 272 |
Power and energy density in the polar cap radio emitter | p. 273 |
Polar cap radio emission | p. 274 |
Radio propagation in the magnetosphere | p. 275 |
Polarisation | p. 275 |
The radio emission mechanism | p. 277 |
Interstellar scintillation and scattering | p. 279 |
A thin-screen model | p. 279 |
Diffraction theory of scintillation | p. 281 |
Thick (extended) scattering screen | p. 282 |
The Fresnel distance | p. 283 |
Strong and weak scintillation | p. 283 |
Distribution in size of the irregularities | p. 284 |
Dynamic scintillation spectra | p. 284 |
The velocity of the scintillation pattern | p. 289 |
Pulse broadening | p. 291 |
Multiple scattering | p. 293 |
Observations of pulse broadening | p. 294 |
Apparent source diameters | p. 296 |
Long-term intensity variations | p. 298 |
The interstellar magnetic field | p. 300 |
Optical and radio observations | p. 300 |
Faraday rotation in pulsars | p. 302 |
The configuration of the local field | p. 303 |
The effect of H II regions | p. 306 |
Achievements and prospects | p. 307 |
The observations and the archive | p. 307 |
The population: birth, death and rejuvenation | p. 309 |
The physics of pulsars | p. 310 |
New telescopes and new horizons | p. 311 |
References | p. 312 |
Index | p. 341 |
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