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Pulsar Electrodynamics

https://doi.org/10.1086/150119
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inferred← citeshttps://doi.org/10.2139/ssrn.6502757openalex-extracted
inferred← citeshttps://doi.org/10.1002/9781394306503.ch2openalex-snapshot
Compact Objects
inferred← citeshttps://doi.org/10.1002/9783527617661.refsopenalex-snapshot
References
inferred← citeshttps://doi.org/10.1002/9783527617982.ch21openalex-snapshot
Propagation of charged particles from the Galactic Center
inferred← citeshttps://doi.org/10.1002/9783527617982.ch52openalex-snapshot
Neutrons, neutrinos, and gamma‐rays from the Galactic Center
inferred← citeshttps://doi.org/10.1002/9783527619054.ch8openalex-snapshot
Outflows and Accretion
inferred← citeshttps://doi.org/10.1002/asna.19702920505openalex-snapshot
Magnetic Neutron Stars. I. Static Field Configurations
inferred← citeshttps://doi.org/10.1002/asna.200385052openalex-snapshot
Neutrons, neutrinos, and gamma-rays from the Galactic Center
inferred← citeshttps://doi.org/10.1002/asna.200385053openalex-snapshot
Propagation of charged particles from the Galactic Center
inferred← citeshttps://doi.org/10.1002/asna.201312024openalex-snapshot
Review of the theory of pulsar‐wind nebulae
inferred← citeshttps://doi.org/10.1002/asna.201312028openalex-snapshot
The stability of strong waves and its implications for pulsar wind shocks
inferred← citeshttps://doi.org/10.1002/asna.201312030openalex-snapshot
High‐energy pulsar models: Developments and new questions
inferred← citeshttps://doi.org/10.1002/asna.201312041openalex-snapshot
Magnetars: The strongest magnets in the Universe
inferred← citeshttps://doi.org/10.1002/asna.201412085openalex-snapshot
Astrophysical implications on the quantized Faraday effect
inferred← citeshttps://doi.org/10.1002/asna.20220092openalex-snapshot
Generation of cosmic rays in pulsar wind nebulae
inferred← citeshttps://doi.org/10.1002/asna.20220111openalex-snapshot
A short review on the pulsar magnetic inclination angles
inferred← citeshttps://doi.org/10.1002/asna.20230153openalex-snapshot
Repeating fast radio bursts reveal the secret of pulsar magnetospheric activity
inferred← citeshttps://doi.org/10.1002/asna.20230176openalex-snapshot
Spin period evolution of Vela pulsar based on the wind emission: Application to the long period radio pulsars GPM J1839 ‐10 (P = 21 min) and GLEAM‐X J1627 (P = 18 min)
inferred← citeshttps://doi.org/10.1002/asna.20240010openalex-snapshot
Non‐symmetrical sparking may hint “zits” on a pulsar surface
inferred← citeshttps://doi.org/10.1002/ctpp.201000031openalex-snapshot
Nonlinear Behavior of Electromagnetic Waves in Ultra‐Relativistic Electron‐Positron Plasmas
inferred← citeshttps://doi.org/10.1002/ctpp.201600076openalex-snapshot
Nonlinear ion‐acoustic cnoidal wave in electron‐positron‐ion plasma with nonextensive electrons
inferred← citeshttps://doi.org/10.1002/ctpp.201700069openalex-snapshot
Modulational instability and generation of envelope solitons in four‐component space plasmas
inferred← citeshttps://doi.org/10.1002/ctpp.201800055openalex-snapshot
Dissipative ion acoustic solitary waves in collisional, magneto‐rotating, non‐thermal electron–positron–ion plasma
inferred← citeshttps://doi.org/10.1002/ctpp.201800132openalex-snapshot
Modulation instability of lower hybrid waves leading to cusp solitons in electron–positron(hole)–ion Thomas Fermi plasma
inferred← citeshttps://doi.org/10.1002/ctpp.70024openalex-snapshot
Influence of Adiabatic Pressure on Kinetic Alfvén Solitary Waves in Magnetized Plasmas With Mixed Electron Populations
inferred← citeshttps://doi.org/10.1002/ctpp.70142openalex-snapshot
Kinetic Alfvén Waves in a Magnetized Dusty Plasma With Polarization Force
inferred← citeshttps://doi.org/10.1002/htj.23027openalex-snapshot
Ion acoustic solitary waves in multicomponent plasmas: Influence of ion drift velocity and nonthermal electrons
inferred← citeshttps://doi.org/10.1002/mma.1670090128openalex-snapshot
A free boundary problem for three‐dimensional harmonic vector fields
inferred← citeshttps://doi.org/10.1002/piuz.19700010503openalex-snapshot
Pulsare
inferred← citeshttps://doi.org/10.1002/piuz.19950260604openalex-snapshot
Exotische Astronomie mit dem Compton‐Observatorium
inferred← citeshttps://doi.org/10.1007/1-4020-3881-x_9openalex-snapshot
Gamma-Ray Emission from Pulsar Outer Magnetospheres
inferred← citeshttps://doi.org/10.1007/1-4020-4085-7_7openalex-snapshot
Magnetically dominated accretion flows (MDAFS) and jet production in the lowhard state
inferred← citeshttps://doi.org/10.1007/10201983_2openalex-snapshot
5.6.2 Radiopulsars
inferred← citeshttps://doi.org/10.1007/3-540-09992-1_101openalex-snapshot
Pulsars
inferred← citeshttps://doi.org/10.1007/3-540-09992-1_103openalex-snapshot
Compact radiation sources in active galactic nuclei
inferred← citeshttps://doi.org/10.1007/3-540-09992-1_105openalex-snapshot
The pulsar magnetosphere
inferred← citeshttps://doi.org/10.1007/3-540-31626-4_3openalex-snapshot
Interacting Binaries: Topics In Close Binary Evolution
inferred← citeshttps://doi.org/10.1007/3-540-31627-2_2openalex-snapshot
Kinetic Plasma Physics
inferred← citeshttps://doi.org/10.1007/3-540-31628-0_2openalex-snapshot
Neutron Stars
inferred← citeshttps://doi.org/10.1007/3-540-31628-0_3openalex-snapshot
Black Holes
inferred← citeshttps://doi.org/10.1007/3-540-44578-1_3openalex-snapshot
Relativistic Superfluid Models for Rotating Neutron Stars
inferred← citeshttps://doi.org/10.1007/3-540-45615-5_5openalex-snapshot
Rotation Powered Pulsars as Sources of High-Energy Particles
inferred← citeshttps://doi.org/10.1007/3-540-46025-x_10openalex-snapshot
Epilogue
inferred← citeshttps://doi.org/10.1007/3-540-56874-3_5openalex-snapshot
Pulsars — the new celestial clocks
inferred← citeshttps://doi.org/10.1007/3540313966_8openalex-snapshot
Stellar Magnetic Fields
inferred← citeshttps://doi.org/10.1007/978-1-4020-2256-2_8openalex-snapshot
Theories of Gamma-Ray Emission from Pulsars
inferred← citeshttps://doi.org/10.1007/978-1-4020-5575-1_2openalex-snapshot
Pulsars as Probes of Relativistic Gravity, Nuclear Matter, and Astrophysical Plasmas
inferred← citeshttps://doi.org/10.1007/978-1-4020-5998-8_15openalex-snapshot
Resonant Compton upscattering in anomalous X-ray pulsars
inferred← citeshttps://doi.org/10.1007/978-1-4020-5998-8_41openalex-snapshot
Thermal X-ray emission from hot polar cap in drifting subpulse pulsars
inferred← citeshttps://doi.org/10.1007/978-1-4020-5998-8_43openalex-snapshot
Impact of neutron star oscillations on the accelerating electric field in the polar cap of pulsar
inferred← citeshttps://doi.org/10.1007/978-1-4020-5998-8_78openalex-snapshot
Force-free magnetosphere of an aligned rotator with differential rotation of open magnetic field lines
inferred← citeshttps://doi.org/10.1007/978-1-4020-5998-8_8openalex-snapshot
Our distorted view of magnetars: application of the resonant cyclotron scattering model
inferred← citeshttps://doi.org/10.1007/978-1-4020-5998-8_83openalex-snapshot
Using XMM-Newton to measure the spectrum of the Vela pulsar and its phase variation
inferred← citeshttps://doi.org/10.1007/978-1-4020-5998-8_88openalex-snapshot
Magnetar corona
inferred← citeshttps://doi.org/10.1007/978-1-4020-6118-9_35openalex-snapshot
An algorithm for solving the pulsar equation
inferred← citeshttps://doi.org/10.1007/978-1-4020-8868-1_10openalex-snapshot
Magnetosphere Structure and the Annular Gap Model of Pulsars
inferred← citeshttps://doi.org/10.1007/978-1-4020-8868-1_8openalex-snapshot
Pulsar Radio Emission Geometry
inferred← citeshttps://doi.org/10.1007/978-1-4612-3936-9_11openalex-snapshot
Pulsars
inferred← citeshttps://doi.org/10.1007/978-1-4614-5782-4_12openalex-snapshot
Ultrarelativistic Component of Astrophysical Plasmas
inferred← citeshttps://doi.org/10.1007/978-1-4614-6455-6_11openalex-snapshot
Pulsar Wind Nebulae as Cosmic Pevatrons: A Current Sheet’s Tale
inferred← citeshttps://doi.org/10.1007/978-1-4615-6758-5_26openalex-snapshot
Stellar Magnetohydrodynamics
inferred← citeshttps://doi.org/10.1007/978-1-4615-6758-5_27openalex-snapshot
Plasma Turbulent Heating and Thermal X-Ray Sources
inferred← citeshttps://doi.org/10.1007/978-1-4615-6758-5_30openalex-snapshot
A Three-Dimensional Relativistic Computation for the Pulsar Magnetosphere
inferred← citeshttps://doi.org/10.1007/978-1-4615-6758-5_32openalex-snapshot
Strong Magnetic Field Effects in the Pulsar Crusts and Atmospheres
inferred← citeshttps://doi.org/10.1007/978-1-4615-8097-3_3openalex-snapshot
Superheavy Elements
inferred← citeshttps://doi.org/10.1007/978-1-4615-9661-5_9openalex-snapshot
Black Holes and the Unification of Asymmetries
inferred← citeshttps://doi.org/10.1007/978-1-4684-6240-1_5openalex-snapshot
Supernova Remnants
inferred← citeshttps://doi.org/10.1007/978-1-4684-6240-1_6openalex-snapshot
Pulsars
inferred← citeshttps://doi.org/10.1007/978-1-4757-0650-5_4openalex-snapshot
High Magnetic Fields in Stars
inferred← citeshttps://doi.org/10.1007/978-1-4757-1149-3_9openalex-snapshot
Black Holes and the Unification of Asymmetries
inferred← citeshttps://doi.org/10.1007/978-1-4939-3547-5_2openalex-snapshot
Electric Current Circuits in Astrophysics
inferred← citeshttps://doi.org/10.1007/978-1-4939-3550-5_7openalex-snapshot
Radio Pulsars
inferred← citeshttps://doi.org/10.1007/978-3-030-19715-5_12openalex-snapshot
Polarimetry of Magnetars and Isolated Neutron Stars
inferred← citeshttps://doi.org/10.1007/978-3-030-24194-0_2openalex-snapshot
Pulsars and Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-3-030-46622-0openalex-snapshot
Superradiance. New Frontiers in Black Hole Physics
inferred← citeshttps://doi.org/10.1007/978-3-030-46622-0_4openalex-snapshot
Black Holes and Superradiant Instabilities
inferred← citeshttps://doi.org/10.1007/978-3-030-46622-0_5openalex-snapshot
Black Hole Superradiance in Astrophysics
inferred← citeshttps://doi.org/10.1007/978-3-030-55231-2_6openalex-snapshot
Neutron Stars, Pulsars, and Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-3-030-85198-9_3openalex-snapshot
The Emission Physics of Millisecond Pulsars
inferred← citeshttps://doi.org/10.1007/978-3-030-85198-9_8openalex-snapshot
Millisecond Magnetars
inferred← citeshttps://doi.org/10.1007/978-3-031-60567-3_6openalex-snapshot
Plasma Processes
inferred← citeshttps://doi.org/10.1007/978-3-031-90186-7_34openalex-snapshot
The Origin of Cosmic Rays: An Enduring Mystery in Physics
inferred← citeshttps://doi.org/10.1007/978-3-319-06761-2_54openalex-snapshot
Hair of Astrophysical Black Holes
inferred← citeshttps://doi.org/10.1007/978-3-319-19000-6_5openalex-snapshot
Black Hole Superradiance in Astrophysics
inferred← citeshttps://doi.org/10.1007/978-3-319-20794-0_46-1openalex-snapshot
Supernova of 1054 and Its Remnant, the Crab Nebula
inferred← citeshttps://doi.org/10.1007/978-3-319-20794-0_73-1openalex-snapshot
Gamma Ray Pulsars: From Radio to Gamma Rays
inferred← citeshttps://doi.org/10.1007/978-3-319-20794-0_95-1openalex-snapshot
Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-3-319-21846-5_46openalex-snapshot
Supernova of 1054 and its Remnant, the Crab Nebula
inferred← citeshttps://doi.org/10.1007/978-3-319-21846-5_73openalex-snapshot
Gamma Ray Pulsars: From Radio to Gamma Rays
inferred← citeshttps://doi.org/10.1007/978-3-319-21846-5_95openalex-snapshot
Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-3-319-44751-3_5openalex-snapshot
Introduction to Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-3-319-63031-1_11openalex-snapshot
Particle Acceleration in Pulsar Wind Nebulae: PIC Modelling
inferred← citeshttps://doi.org/10.1007/978-3-319-63031-1_8openalex-snapshot
Radiative Models of Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-3-319-97538-2_7openalex-snapshot
Introduction to Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-3-319-97616-7_2openalex-snapshot
Strongly Magnetized Pulsars: Explosive Events and Evolution
inferred← citeshttps://doi.org/10.1007/978-3-540-76965-1_15openalex-snapshot
Pulsar Emission: Where to Go
inferred← citeshttps://doi.org/10.1007/978-3-540-76965-1_18openalex-snapshot
High Energy Emission from Pulsars and Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-3-540-76965-1_19openalex-snapshot
High-energy Emission from the Polar Cap and Slot Gap
inferred← citeshttps://doi.org/10.1007/978-3-540-76965-1_2openalex-snapshot
Radio Emission Properties of Pulsars
inferred← citeshttps://doi.org/10.1007/978-3-540-76965-1_20openalex-snapshot
Physics of Drifting Sub-pulses in Radio Pulsars
inferred← citeshttps://doi.org/10.1007/978-3-540-76965-1_4openalex-snapshot
Intermittent Pulsars
inferred← citeshttps://doi.org/10.1007/978-3-642-14734-0_5openalex-snapshot
Final Stages of Stellar Evolution
inferred← citeshttps://doi.org/10.1007/978-3-642-17251-9_10openalex-snapshot
What Pulsar High-Energy Emission Model Survives?
inferred← citeshttps://doi.org/10.1007/978-3-642-17251-9_12openalex-snapshot
Modeling of γ-ray Pulsar Light Curves from Force-Free Magnetosphere
inferred← citeshttps://doi.org/10.1007/978-3-642-17251-9_13openalex-snapshot
A Tale of Two Current Sheets
inferred← citeshttps://doi.org/10.1007/978-3-642-17251-9_16openalex-snapshot
Modelling the Growing Population of γ-ray Millisecond Pulsars
inferred← citeshttps://doi.org/10.1007/978-3-642-17251-9_24openalex-snapshot
Activated Magnetospheres of Magnetars
inferred← citeshttps://doi.org/10.1007/978-3-642-17251-9_8openalex-snapshot
Emission from the Polar Cap and Slot Gap
inferred← citeshttps://doi.org/10.1007/978-3-642-17251-9_9openalex-snapshot
Gamma-ray emission and pair creation of outer gap
inferred← citeshttps://doi.org/10.1007/978-3-642-19627-0_2openalex-snapshot
Neutron Stars
inferred← citeshttps://doi.org/10.1007/978-3-642-19627-0_8openalex-snapshot
RRATs: An Overview
inferred← citeshttps://doi.org/10.1007/978-3-642-35410-6_1openalex-snapshot
Prologue: γ-Rays from Star-Forming Regions, a Historical Perspective
inferred← citeshttps://doi.org/10.1007/978-3-642-36134-0_3openalex-snapshot
Sources of GeV Photons and the Fermi Results
inferred← citeshttps://doi.org/10.1007/978-3-642-39596-3_5openalex-snapshot
Jets
inferred← citeshttps://doi.org/10.1007/978-3-642-49290-7_14openalex-snapshot
Radio Sources, Quasars, Pulsars, X Ray-, Gamma Ray-Sources, Cosmic Radiation
inferred← citeshttps://doi.org/10.1007/978-3-642-83527-8_7openalex-snapshot
Acoustic Phenomena in Strong Gravitational and Magnetic Fields
inferred← citeshttps://doi.org/10.1007/978-3-642-96178-6_5openalex-snapshot
Supernova Remnants
inferred← citeshttps://doi.org/10.1007/978-3-642-96178-6_6openalex-snapshot
Pulsars
inferred← citeshttps://doi.org/10.1007/978-3-662-04593-0_6openalex-snapshot
Gamma-Ray Pulsars
inferred← citeshttps://doi.org/10.1007/978-3-662-11188-8_4openalex-snapshot
Nuclear Astrophysics and High Energy Particles
inferred← citeshttps://doi.org/10.1007/978-3-662-21642-2_4openalex-snapshot
Nuclear Astrophysics and High Energy Particles
inferred← citeshttps://doi.org/10.1007/978-3-662-62110-3_2openalex-snapshot
General Relativity Measurements from Pulsars
inferred← citeshttps://doi.org/10.1007/978-3-7091-8498-1_17openalex-snapshot
Cosmic Gamma Radiation
inferred← citeshttps://doi.org/10.1007/978-4-431-67029-2_14openalex-snapshot
Particle Acceleration Mechanisms in Astrophysics
inferred← citeshttps://doi.org/10.1007/978-94-007-5615-1_12openalex-snapshot
Black Holes and Neutron Stars
inferred← citeshttps://doi.org/10.1007/978-94-009-0171-1_18openalex-snapshot
Pulsars as Gamma Ray Sources: Nebular Shocks and Magnetospheric Gaps
inferred← citeshttps://doi.org/10.1007/978-94-009-0265-7_18openalex-snapshot
Numerical Simulation of Plasma Flow in the Magnetosphere of an Axisymmetric Rotator
inferred← citeshttps://doi.org/10.1007/978-94-009-0515-3_13openalex-snapshot
2D Relativistic Pulsar Winds From Rapidly Rotating Neutron Stars
inferred← citeshttps://doi.org/10.1007/978-94-009-0545-0_19openalex-snapshot
Plerionic Supernova Remnants
inferred← citeshttps://doi.org/10.1007/978-94-009-1673-9_13openalex-snapshot
Magnetohydrodynamic Jets and Winds from Accretion Disks
inferred← citeshttps://doi.org/10.1007/978-94-009-2273-0_56openalex-snapshot
Self-Consistent Modelling of Pulsar Magnetospheres
inferred← citeshttps://doi.org/10.1007/978-94-009-2401-7_13openalex-snapshot
Jets and Magnetic Fields
inferred← citeshttps://doi.org/10.1007/978-94-009-2941-8_1openalex-snapshot
Quasi-Steady Outflows from Astrophysical Objects: Complementary Views from Different Experiences
inferred← citeshttps://doi.org/10.1007/978-94-009-2949-4_18openalex-snapshot
Electrodynamics of the Central Regions of Active Galactic Nuclei
inferred← citeshttps://doi.org/10.1007/978-94-009-3823-6_6openalex-snapshot
Observations of Pulsars
inferred← citeshttps://doi.org/10.1007/978-94-009-3823-6_7openalex-snapshot
Energetic Radiation from Magnetized Neutron Stars
inferred← citeshttps://doi.org/10.1007/978-94-009-3913-4_100openalex-snapshot
Cygnus X-3 and other Ultra-High-Energy γ-Ray Sources
inferred← citeshttps://doi.org/10.1007/978-94-009-3913-4_24openalex-snapshot
Neutron Star Coupling to its Environment
inferred← citeshttps://doi.org/10.1007/978-94-009-4025-3_12openalex-snapshot
Pulsars as Cosmic Ray Particle Accelerators — New Results on the Dynamics of Protons in Vacuum Fields
inferred← citeshttps://doi.org/10.1007/978-94-009-4630-9_19openalex-snapshot
Electrodynamical Synchronization of AM Herculis-Type Stars
inferred← citeshttps://doi.org/10.1007/978-94-009-6520-1_49openalex-snapshot
Accretion Disk Electrodynamics
inferred← citeshttps://doi.org/10.1007/978-94-009-7208-7_9openalex-snapshot
Gamma-Ray Pulsars in the MeV Region
inferred← citeshttps://doi.org/10.1007/978-94-009-7231-5_45openalex-snapshot
X-Ray Observations of Crab-Like Supernova Remnants
inferred← citeshttps://doi.org/10.1007/978-94-009-7766-2_30openalex-snapshot
Active Galactic Nuclei and Particle Acceleration in Accretion Disks Around Massive Black Holes
inferred← citeshttps://doi.org/10.1007/978-94-009-8475-2_28openalex-snapshot
Particle Acceleration by Pulsars
inferred← citeshttps://doi.org/10.1007/978-94-010-0904-1_30openalex-snapshot
Radio Pulsars — What Is to Be Done
inferred← citeshttps://doi.org/10.1007/978-94-010-1007-8_20openalex-snapshot
NP Black Holes as High Energy Gamma-Ray Sources
inferred← citeshttps://doi.org/10.1007/978-94-010-1789-3_36openalex-snapshot
Is Jupiter’s Magnetosphere Like a Pulsar’s or Earth’s?
inferred← citeshttps://doi.org/10.1007/978-94-010-1812-8_14openalex-snapshot
Collapsed Stars, Pulsars and the Origin of Cosmic Rays
inferred← citeshttps://doi.org/10.1007/978-94-010-2138-8_11openalex-snapshot
Superfluidity in Neutron Stars
inferred← citeshttps://doi.org/10.1007/978-94-010-2138-8_17openalex-snapshot
Pulsar Observations and Neutron Star Models
inferred← citeshttps://doi.org/10.1007/978-94-010-2166-1_45openalex-snapshot
On the Formation of Wisps in the Crab Nebula
inferred← citeshttps://doi.org/10.1007/978-94-010-2211-8_47openalex-snapshot
Summary
inferred← citeshttps://doi.org/10.1007/978-94-010-2585-0_14openalex-snapshot
Pulsars and X-ray Sources
inferred← citeshttps://doi.org/10.1007/978-94-010-2658-1_4openalex-snapshot
A Cosmochemical View of Cosmic Rays and Solar Particles
inferred← citeshttps://doi.org/10.1007/978-94-010-3087-8_28openalex-snapshot
Polarization of Pulsars
inferred← citeshttps://doi.org/10.1007/978-94-010-3087-8_41openalex-snapshot
The Secular Behavior of X-ray and Radio Emission from Supernova Remnants
inferred← citeshttps://doi.org/10.1007/978-94-010-3087-8_49openalex-snapshot
General Relativistic Theory of Rotating Neutron Stars — A Review
inferred← citeshttps://doi.org/10.1007/978-94-010-3087-8_54openalex-snapshot
Periodicity and Luminosity of the ‘Pulsar’ Model of Quasars
inferred← citeshttps://doi.org/10.1007/978-94-010-3087-8_57openalex-snapshot
Young Pulsars — Pulsed Neutron Sources
inferred← citeshttps://doi.org/10.1007/978-94-010-3087-8_58openalex-snapshot
Relationship between Pulsar and Nebula
inferred← citeshttps://doi.org/10.1007/978-94-010-3087-8_60openalex-snapshot
Physical Processes and Parameters in the Magnetosphere of NP 0532
inferred← citeshttps://doi.org/10.1007/978-94-010-3087-8_62openalex-snapshot
Maser Theory of Pulsar Radiation
inferred← citeshttps://doi.org/10.1007/978-94-010-3087-8_69openalex-snapshot
Pulsar (and X-Star) Emission from the Magnetosphere of a Collapsed Star
inferred← citeshttps://doi.org/10.1007/978-94-010-3102-8_2openalex-snapshot
Pulsars (Theoretical Considerations)
inferred← citeshttps://doi.org/10.1007/978-94-010-3311-4_35openalex-snapshot
Radio, Optical and X-Ray Emission from Pulsars
inferred← citeshttps://doi.org/10.1007/978-94-011-0159-2_17openalex-snapshot
Radio Pulsar Slowdown
inferred← citeshttps://doi.org/10.1007/978-94-011-0159-2_28openalex-snapshot
OSSE Limits on Pulsar Gamma-Ray Emission
inferred← citeshttps://doi.org/10.1007/978-94-011-1014-3_51openalex-snapshot
Electric Gaps in Pulsar Magnetospheres
inferred← citeshttps://doi.org/10.1007/978-94-011-1014-3_52openalex-snapshot
Radiative Properties of Pulsar Magnetospheres
inferred← citeshttps://doi.org/10.1007/978-94-011-1110-2_18openalex-snapshot
Cosmical Magnetism
inferred← citeshttps://doi.org/10.1007/978-94-011-1924-5_70openalex-snapshot
Mechanisms of Jet Formation
inferred← citeshttps://doi.org/10.1007/978-94-011-2704-2_21openalex-snapshot
Some Problems in the Theory of Isolated Pulsars
inferred← citeshttps://doi.org/10.1007/978-94-011-3158-2_14openalex-snapshot
The Effect of Relativistic Particle Beams on the Evolution of Supernova Envelopes: Self-Consistent Solutions
inferred← citeshttps://doi.org/10.1007/978-94-011-3536-8_6openalex-snapshot
Neutron Star Plate Tectonics
inferred← citeshttps://doi.org/10.1007/978-94-011-4203-8_31openalex-snapshot
Coherent Emission Mechanisms In Radio Pulsars
inferred← citeshttps://doi.org/10.1007/978-94-011-7912-6_11openalex-snapshot
Propagation of Large Amplitude Pulsar Waves
inferred← citeshttps://doi.org/10.1007/978-94-011-7912-6_19openalex-snapshot
Radio Observational Constraints on Pulsar Emission Mechanisms
inferred← citeshttps://doi.org/10.1007/978-94-011-7912-6_2openalex-snapshot
Structure of the Pulsar Magnetosphere
inferred← citeshttps://doi.org/10.1007/978-94-011-7912-6_21openalex-snapshot
Pulse Emission from the Light Cylinder
inferred← citeshttps://doi.org/10.1007/978-94-011-7912-6_3openalex-snapshot
The Axially Symmetric Wind Magnetosphere
inferred← citeshttps://doi.org/10.1007/978-94-011-7912-6_9openalex-snapshot
Electric Field Near a Rotating Neutron Star
inferred← citeshttps://doi.org/10.1007/978-94-015-8557-6_2openalex-snapshot
Gravitoelectrodynamics
inferred← citeshttps://doi.org/10.1007/978-94-015-9139-3_1openalex-snapshot
The History of Neutron Stars: From Early Speculations to Current Problems
inferred← citeshttps://doi.org/10.1007/978-94-015-9723-4_30openalex-snapshot
Massive Star Population Synthesis of Starbursts
inferred← citeshttps://doi.org/10.1007/978-94-017-0403-8_11openalex-snapshot
Bare Strange Quark Stars: Formation and Emission
inferred← citeshttps://doi.org/10.1007/978-94-024-1292-5_5openalex-snapshot
Electrodynamics of Pulsar Magnetospheres
inferred← citeshttps://doi.org/10.1007/978-94-024-1292-5_6openalex-snapshot
Modelling Jets, Tori and Flares in Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-981-16-4544-0_102-1openalex-snapshot
Isolated Neutron Stars
inferred← citeshttps://doi.org/10.1007/978-981-16-4544-0_105-1openalex-snapshot
Fundamental Physics with Neutron Stars
inferred← citeshttps://doi.org/10.1007/978-981-16-4544-0_128-1openalex-snapshot
Fast Radio Bursts
inferred← citeshttps://doi.org/10.1007/978-981-16-4544-0_157-1openalex-snapshot
Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-981-19-6960-7_102openalex-snapshot
Isolated Neutron Stars
inferred← citeshttps://doi.org/10.1007/978-981-19-6960-7_105openalex-snapshot
Fundamental Physics with Neutron Stars
inferred← citeshttps://doi.org/10.1007/978-981-19-6960-7_128openalex-snapshot
Fast Radio Bursts
inferred← citeshttps://doi.org/10.1007/978-981-19-6960-7_157openalex-snapshot
Pulsar Wind Nebulae
inferred← citeshttps://doi.org/10.1007/978-981-97-8522-3_17openalex-snapshot
Black Hole-Neutron Star Binaries
inferred← citeshttps://doi.org/10.1007/bf00155751openalex-snapshot
On practical representation of magnetic field
inferred← citeshttps://doi.org/10.1007/bf00167500openalex-snapshot
Gamma-ray pulsars in the MeV region
inferred← citeshttps://doi.org/10.1007/bf00490395openalex-snapshot
Wie aussichtsreich ist die Suche nach Gamma-Pulsaren?
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