منابع مشابه
Energetic Young Radio Pulsars
Young radio pulsars shed vast amounts of rotational energy, sometimes as high as 100,000 times the total energy loss rate from the sun. The wide range of phenomena resulting from this energy loss include: glitches, timing noise, jets, bow shocks, bullets and plerions and are be reviewed from an observational perspective. Past and proposed surveys for young radio pulsars are summarised along wit...
متن کاملProfile and polarization characteristics of energetic pulsars
In this paper we compare the characteristics of pulsars with a high spin-down energy loss rate (Ė) against those with a low Ė. We show that the differences in the total intensity pulse morphology between the two classes are in general rather subtle. A much more significant difference is the fractional polarization which is very high for high Ė pulsars and low for low Ė pulsars. The Ė at the tra...
متن کاملRecent Discoveries of Energetic Young Radio Pulsars
The observed population of young radio pulsars has grown substantially in recent years due to a combination of large-scale surveys and deep targeted searches. Many of the pulsars are associated with supernova remnants and/or unidentified gamma-ray sources. This review summarises the state of play and looks ahead to likely advances in the near future.
متن کاملShocks and Wind Bubbles Around Energetic Pulsars
The Crab Nebula demonstrates that neutron stars can interact with their environments in spectacular fashion, their relativistic winds generating nebulae observable across the electromagnetic spectrum. At many previous conferences, astronomers have discussed, debated and puzzled over the complicated structures seen in the Crab, but have been limited to treating most other pulsar wind nebulae (PW...
متن کاملObservations of Energetic High Magnetic Field Pulsars with the Fermi Large Area Telescope
We report the detection of γ-ray pulsations from the high-magnetic-field rotation-powered pulsar PSR J1119−6127 using data from the Fermi Large Area Telescope. The γ-ray light curve of PSR J1119−6127 shows a single, wide peak offset from the radio peak by 0.43± 0.02 in phase. Spectral analysis suggests a power law of index 1.0± 0.3 −0.2 with an energy cut-off at 0.8± 0.2 +2.0 −0.5GeV. The first...
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ژورنال
عنوان ژورنال: Proceedings of the International Astronomical Union
سال: 2017
ISSN: 1743-9213,1743-9221
DOI: 10.1017/s1743921317009498