On the method of estimating emission altitude from relativistic phase shift in pulsars

Abstract

In the preprint astro-ph/0411161 (hereafter G04b), the term -(Omega r/c) sin(theta')cos(Theta) is missing in the equation (13) for cos(psi). So, in this is supplementary preprint I give the corrected expression for cos(psi) and the revised derivation of aberration phase shift.

arXiv comment4 pages, Corrections to astro-ph/0411161

References in corpus (6)

• Understanding the radio emission geometry of PSR B0329+54
• On the methods of determining the radio emission geometry in pulsar magnetospheres
• Understanding the radio emission geometry of multi-component radio pulsars from retardation and aberration effects
• Polarization Sweeps in Rotation Powered Pulsars
• Rotational sweepback of magnetic field lines in geometrical models of pulsar radio emission
• Pulsar Radio Emission Altitude from Curvature Radiation

Cited by in corpus (21)

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• Constraints on viewing geometries from radio observations of $\gamma$-ray-loud pulsars using a novel method
• High frequency observations of southern pulsars
• Curvature Radiation in Rotating Pulsar Magnetosphere
• On the aberration-retardation effects in pulsars
• Visibility of pulsar emission: motion of the visible point
• The annular gap model for gamma-ray emission from young and millisecond pulsars
• Relativistic model on pulsar radio emission and polarization
• Neutron Star Physics in the Square Kilometer Array Era : An Indian Perspective
• Dynamics of Charged Particles in the Radio Emission Region of Pulsar Magnetosphere
• Modeling the frequency-dependence of radio beams for cone-dominant pulsars
• Size of the Vela Pulsar's Emission Region at 18 cm Wavelength
• Absolute emission altitude of pulsars: PSRs B1839+09, B1916+14 and B2111+46
• Influence of the polar cap current on pulsar polarization
• Lower bounds of altitudes for pulsar $\gamma$-ray radiation
• Role of rotation and polar cap current on pulsar radio emission and polarization
• Understanding the effects of geometry and rotation on pulsar intensity profiles
• Role of Fan Beam Model in Population Synthesis of Isolated Radio Pulsars
• Polarized radio emission of RRAT J1854+0306
• The Effects of Finite Emission Height in Precision Pulsar Timing
• Pulsars as Fantastic Objects and Probes