Neutron Stars and Pulsars
Neutron stars are the most compact astronomical objects in the universe which are accessible by direct observation. Studying neutron stars means studying physics in regimes unattainable in any terrestrial laboratory. Understanding their observed complex phenomena requires a wide range of scientific...
| Συγγραφή απο Οργανισμό/Αρχή: | |
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| Άλλοι συγγραφείς: | |
| Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
| Γλώσσα: | English |
| Έκδοση: |
Berlin, Heidelberg :
Springer Berlin Heidelberg,
2009.
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| Σειρά: | Astrophysics and Space Science Library,
357 |
| Θέματα: | |
| Διαθέσιμο Online: | Full Text via HEAL-Link |
Πίνακας περιεχομένων:
- Radio Pulsar Statistics
- Radio Emission Properties of Pulsars
- Rotating Radio Transients
- Intermittent Pulsars
- The Double Pulsar: A Unique Lab for Relativistic Plasma Physics and Tests of General Relativity
- X-Ray Emission from Pulsars and Neutron Stars
- Isolated Neutron Stars: The Challenge of Simplicity
- Millisecond Pulsars in Globular Clusters and the Field
- Theory of Radiative Transfer in Neutron Star Atmospheres and Its Applications
- Neutron Star Interiors and the Equation of State of Superdense Matter
- Neutron Star Cooling: I
- Neutron Star Cooling: II
- Turning Points in the Evolution of Isolated Neutron Stars'Magnetic Fields
- Pulsar Spin, Magnetic Fields, and Glitches
- Pulsar Emission: Where to Go
- The Theory of Pulsar Winds and Nebulae
- Implications of HESS Observations of Pulsar
- High Energy Emission from Pulsars and Pulsar Wind Nebulae
- High-energy Emission from the Polar Cap and Slot Gap
- Physics of Drifting Sub-pulses in Radio Pulsars
- Soft Gamma-Ray Repeaters and Magnetars
- X-Ray Polarimetry and Its Potential Use for Understanding Neutron Stars
- GeV Gamma-Ray Pulsar Detection
- Gravitational Waves from Spinning Neutron Stars.
