Young Neutron Stars and Their Environments

By F. Camilo, B. Gaensler. 2004

291 citations recorded by the source corpus.

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Citations in the corpus

On the Polar Caps of the Three Musketeers (2004, methodology): “Multicolor photometry, which is available for Geminga and PSR B0656+ 14, shows that their NUV magnitudes are broadly compatible with the extrapolations of their X-ray blackbody emissions, while a power-law–like excess is apparent in the optical/NIR (Mignani et al. 2004 and references therein).”
Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields (2004, background): “The greatest fractional decrease occurs during the transition from hydrogen depletion to helium ignition (Table 1, Fig.”
On the force‐free magnetosphere of an aligned rotator (2005, background): “…debated (see e.g. Smith et al. 2001; Pétri et al. 2002), where there are several separated clouds of charged particles near the NS and no particle outflow, however there are indications that such configuration is unstable against diocotron instability (Spitkovsky & Arons 2002; Spitkovsky 2004).”
The subpulse modulation properties of pulsars at 21 cm (2005, background): “For PSR B1839−04 we observe that the two components have mirrored drift bands (i.e. the components drift in phase) like PSR J0815+09, something we do not know for the other pulsars.”
Dissipation of Magnetohydrodynamic Waves on Energetic Particles: Impact on Interstellar Turbulence and Cosmic-Ray Transport (2005, background): “We note that the adapted source distribution5 is flatter than the distribution of SNR (Case & Bhattacharya 1998) and pulsars (Lorimer 2004).”