The Very Young Radio Pulsar J1357-6429
arXiv:astro-ph/0406528 · doi:10.1086/423620
Abstract
We report the discovery of a radio pulsar with a characteristic age of 7300 years, making it one of the 10 apparently youngest Galactic pulsars known. PSR J1357-6429, with a spin period of P = 166 ms and spin-down luminosity of 3.1e36 ergs/s, was detected during the Parkes multibeam survey of the Galactic plane. We have measured a large rotational glitch in this pulsar, with Delta P/P = -2.4e-6, similar in magnitude to those experienced occasionally by the Vela pulsar. At a nominal distance of only ~ 2.5 kpc, based on the measured free electron column density of 127 pc/cc and the electron distribution model of Cordes & Lazio, this may be, after the Crab, the nearest very young pulsar known. The pulsar is located near the radio supernova remnant candidate G309.8-2.6.
arXiv commentAccepted for publication in ApJ Letters; 6 pages, 2 included EPS figures
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Cited by in corpus (23)
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- Avalanche dynamics of radio pulsar glitches
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- Constraints on the Galactic Population of TEV Pulsar Wind Nebulae Using Fermi Large Area Telescope Observations
- The gas-to-extinction ratio and the gas distribution in the Galaxy
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- Discovery of the source HESS J1356-645 associated with the young and energetic PSR J1357-6429
- First X-ray observations of the young pulsar J1357-6429
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- Discovery of X-ray emission from the young radio pulsar PSR J1357-6429
- GeV gamma-ray emission from pulsar wind nebula HESS J1356-645 with Fermi-LAT
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- High-time Resolution Astrophysics and Pulsars
- Observations of PSR J1357-6429 at 2.1 GHz with the Australia Telescope Compact Array
- Suzaku Observations of the old pulsar wind nebula candidate HESS J1356-645